The galaxy presents as a primarily smooth object with a concentrated central region. It exhibits a mildly elliptical morphology, appearing neither perfectly round nor highly elongated. There is evidence of possible minor disturbances or interactions, although the overall structure is largely undisturbed. The color profile suggests a population of older stars, with a redder hue dominating the observed light. There may be evidence of a merger based on the slight irregular shape. Star formation is likely subdued in the main body of the galaxy.
