The galaxy presents as a relatively smooth, elliptical-like morphology. It appears to be fairly lenticular, exhibiting a concentrated, bright central bulge that is slightly elongated along the major axis. There are no visible spiral arm structures or significant dust lanes. The color profile suggests an older stellar population, with a yellowish-white hue dominating the central region, indicative of evolved stars. The outer regions appear to be more diffuse and subtly bluer, perhaps due to a small amount of recent star formation, though this is not definitive from the image alone. There is no evidence of tidal tails or other major disturbances that would indicate a recent or ongoing merger event, though a very slight asymmetry on one side hints at a possible minor interaction. The galaxy is reasonably well-defined but lacks intricate details in this image.
