The galaxy presents as a relatively compact object with a generally smooth morphology. There is a subtle central concentration of light, suggesting a possible core or bulge region. The overall shape appears to be roughly elliptical, with the isophotes appearing somewhat rounded, but the minor axis seems to be slightly shorter than the major axis. The color gradient across the galaxy is subtle, but it appears to be redder in the center and bluer toward the edges. There are no distinct spiral arms or prominent dust lanes visible. The image indicates that this is an older stellar population, or a galaxy with a low rate of ongoing star formation. There is no evidence of any major tidal disturbances, or ongoing mergers.
