The galaxy appears as a relatively smooth, elliptical-like structure. There is a hint of a disk, but the overall impression is of a system dominated by an older stellar population. The galaxy has an apparent moderate concentration of light towards the center. The color is generally redder overall, indicative of a population of older stars, consistent with a more passive or quiescent galaxy with a modest rate of star formation. There is evidence of minor disturbance and possible tidal features, suggesting potential interaction with other galaxies. About 80% of the galaxy's shape appears to be round with the remainder appearing to be in between round and cigar shaped. Approximately 25% of the galaxy appears to be in a merging state with another galaxy.
