The galaxy presents a smooth, elliptical morphology. A concentrated central bulge is apparent, exhibiting a yellowish hue, likely indicating an older stellar population. Extending outward from the core is a fainter, more diffuse halo or disk. This outer region displays hints of bluer colors, possibly suggesting the presence of younger, hotter stars, and indicating some level of ongoing or recent star formation within the galaxy, albeit at a modest rate. There are no distinct spiral arms or prominent dust lanes visible. The overall structure suggests a system that is primarily spheroidal, although not perfectly round. There is no obvious evidence of major mergers or significant tidal disturbances. Slight asymmetry is present in the outer regions, suggestive of a minor interaction.
