The galaxy presents a smooth, largely featureless morphology. Its overall shape appears elliptical, with a high degree of circularity. The light distribution is concentrated towards the center, exhibiting a bright core that gradually fades into the surrounding halo. There is some variation in color, with the central region displaying a bluer hue, possibly indicative of a younger stellar population or ongoing star formation activity, however the levels are very low. The outer regions transition towards redder tones, suggesting the presence of older stars. There is no evidence of spiral arms, prominent dust lanes, or tidal features to indicate any recent major merger events or significant ongoing interactions. The overall appearance suggests a relatively evolved system.
