The galaxy presents a relatively smooth, elliptical morphology. There is little evidence of spiral arms or significant dust lanes. The color profile appears to be fairly uniform across the galaxy, trending towards bluer hues at the center. It appears to be moderately luminous, with a concentrated central region indicative of a bulge, which is surrounded by a slightly fainter, more diffuse halo. The overall shape is somewhat rounded, lacking any apparent strong tidal distortions or signs of recent major merger events. Faint color gradients could suggest some ongoing, though subdued, star formation activity. There are no obvious features suggestive of an active galactic nucleus.
