The galaxy presents a morphology that is neither purely elliptical nor a well-defined spiral. It exhibits a central bulge that is luminous and appears yellowish-white, indicative of an older stellar population. Fainter, diffuse structures extend from the central region, suggesting the presence of a disk or irregular arms. The overall shape is more elongated than circular, tending towards an in-between form. There are hints of minor distortions, such as faint asymmetric features emanating from the galaxy, potentially caused by interactions. The galaxy exhibits relatively red colors, likely indicating a population dominated by older stars and/or significant dust obscuration.
