The galaxy presents an elliptical morphology, appearing relatively smooth in structure. A central bulge is distinctly visible, exhibiting a yellowish hue, suggestive of an older stellar population. Surrounding the bulge is a fainter, bluer halo or disk-like structure, possibly indicating a small amount of on-going star formation, although the overall star formation rate appears to be low. The galaxy's shape appears somewhat elongated, not perfectly spherical, leaning towards an intermediate roundedness. There are subtle indications of minor disturbances in the galaxy's outer regions, but no major signs of a significant merger or tidal interactions with other galaxies. The galaxy exhibits an overall concentrated light profile, with the majority of the light emanating from the central bulge.
