The galaxy presents as a relatively smooth, elliptical-like structure. Its core appears as a concentrated, bright yellow hue, indicative of a population of older stars. The outer regions gradually fade into a less intense, more reddish color, further supporting the presence of an aging stellar population. There is minimal indication of spiral arms or prominent dust lanes. The overall morphology suggests that the galaxy may be in a relatively quiescent state, with limited ongoing star formation. There may be a slight asymmetry in the surrounding region of the galaxy, potentially indicating a previous minor interaction with another galaxy, but no clear signs of active merging or major disturbances can be discerned.
