The galaxy appears as a slightly elongated, lenticular structure, approximately 2.4 kpc across. It displays a generally smooth, centrally concentrated luminosity profile, with minimal discernible spiral arm structure or dust lanes. There is a hint of a flattened disk shape, but the morphology is predominantly spheroid-like. The galaxy's color is slightly yellowish, suggesting a population of older stars and a low rate of ongoing star formation. There is no evidence of significant morphological disturbance or ongoing merging activity.
