The galaxy presents a predominantly smooth morphology, suggesting an elliptical classification, although with some disklike features. It appears relatively round in shape, with a concentrated central bulge exhibiting a yellowish hue. This may indicate an older stellar population within the bulge. The outer regions of the galaxy show a slightly bluer color, which may imply the presence of a younger stellar population or ongoing star formation activity. There may be a very slight distortion of the galaxy shape, and possible tidal features. This indicates possible past or ongoing gravitational interactions with another galaxy.
