The galaxy exhibits a morphology that is neither purely elliptical nor a well-defined spiral. There is evidence of some internal structure, suggestive of a possible disk component or tidal features. The color profile is not uniform; a bluer region is apparent to the Northwest, while a more reddened area is located to the Southeast. This color variation may be indicative of differing stellar populations or dust obscuration within the galaxy. There is indication of a possible minor interaction with a smaller body to the Southwest. This system may be in the process of merging or experiencing a gravitational disturbance. The overall size appears relatively compact.