The galaxy presents a generally smooth, elliptical morphology. The central region exhibits a high surface brightness, appearing nearly uniform and intensely luminous. Moving outwards from the core, the luminosity gradually decreases, forming a diffuse halo around the brighter center. The shape of the galaxy appears elongated, with the major axis extending significantly further than the minor axis, indicative of an elliptical galaxy with some degree of flattening. There are faint hints of structure within the extended halo, possibly representing unresolved stellar populations or dust lanes. However, there is no clear evidence of spiral arms, a central bar, or other prominent features typically associated with spiral galaxies. The overall color is slightly redder in the central regions, shifting towards a bluer hue in the outer halo, which could suggest differences in the age and composition of stellar populations, with older, redder stars dominating the core and younger, bluer stars residing in the outer regions. There are some signs of minor disturbances in the halo, but nothing indicating a major merger event.
