The galaxy presents as a somewhat diffuse object, with an overall smooth appearance punctuated by some features. The light distribution appears moderately concentrated towards the center. The object exhibits an elliptical shape, appearing close to round. Evidence suggests some degree of ongoing or recent interaction, possibly a merger or tidal disturbance, based on the disturbed morphology. The galaxy is moderately luminous, indicative of a substantial stellar population. There are no apparent strong spiral arm structures. The colors suggest a mix of stellar populations, with some indication of older stars contributing to the overall light. Star formation may be present but is not particularly dominant in the galaxy's overall appearance.
