The galaxy presents a generally elliptical morphology, appearing as a somewhat flattened spheroid of light. It displays a radial intensity gradient, with a bright, concentrated core diminishing outwards to a fainter, more diffuse halo. The primary color is a warm yellow-orange hue, suggesting an older stellar population. A subtle asymmetry in the extended halo may indicate past or ongoing interactions. There is little evidence of prominent spiral arms or significant dust lanes. The overall smoothness of the light distribution points toward a galaxy with a bulge-dominated structure.
