The galaxy in question appears to be a relatively compact, elliptical or lenticular system. It exhibits a generally smooth, diffuse light profile without prominent spiral arms or a distinct central bulge. The overall shape is approximately round, with a minor suggestion of elongation. The galaxy's light distribution suggests an older stellar population, with no obvious regions of intense star formation or blue emission. There is faint evidence of a possible minor disturbance or tidal feature in the galaxy's halo, but it is extremely subtle. The galaxy does not appear to be undergoing a major merger. There may be a minor interaction with a companion galaxy based on the slight disturbance. It exhibits a redder overall color, typical of galaxies dominated by evolved stars.
