The galaxy appears to be a relatively smooth, elliptical galaxy with a centrally concentrated bulge. There is minimal evidence of distinct spiral arms or prominent dust lanes. The light distribution suggests a primarily older stellar population, indicated by the redder color. The overall structure is somewhat round, displaying an intermediate ellipticity. There appears to be little to no significant tidal disturbance or merging activity evident in the image. The star formation rate appears to be relatively low, implying a passively evolving system. The estimated size of the galaxy is a few kiloparsecs, placing it within the range of a typical dwarf galaxy.
