The galaxy presents as a relatively smooth object with a mostly elliptical morphology. A distinct, brighter central bulge is apparent, surrounded by a less luminous halo. There is a slight elongation to the galaxy's overall shape, but no obvious spiral arm structures are visible. The color distribution shows a concentration of yellow-orange hues in the center, suggesting an older stellar population. A faint bluish tail-like extension emanates from one side of the galaxy, indicating a potential tidal interaction or ram pressure stripping. There are no signs of ongoing major mergers or significant disturbances to the galaxy's overall structure.
