The galaxy presents a largely smooth and centrally concentrated light distribution. There is no readily discernible spiral structure or prominent disk. The overall shape appears close to circular, with minimal elongation or asymmetry. A faint, diffuse halo might be present, extending slightly beyond the brighter central region, but this is subtle. The galaxy exhibits a yellow-red hue, suggesting an older stellar population and relatively low ongoing star formation. There's no obvious indication of strong tidal interactions or recent merger events. Small disturbances seem to be present as a faint, blurred formation near the edges of the galaxy's light. The galaxy's magnitude indicates it is a relatively bright and massive object at its distance.
