The galaxy presents as a single, relatively smooth object with a concentrated central region. It exhibits an elliptical morphology, with the bulk of its light concentrated towards the center. A slight elongation is visible, deviating from a perfect circular shape.

The color profile suggests a relatively older stellar population, with a dominance of redder hues. This potentially indicates a reduced rate of ongoing star formation. The lack of distinct blue regions, typically associated with young, hot stars, supports this interpretation.

There is some irregular structure present. It is unclear if this is an ongoing interaction with another galaxy, but the slight asymmetry does suggest some form of external influence.

