The galaxy presents a primarily smooth morphology. The light distribution appears concentrated towards the center, suggesting a prominent bulge. A faint disk component may be present, though this is not distinct due to the smoothness of the overall light profile. There is no strong evidence of spiral arms or other features. The galaxy's shape is roughly circular, although it appears slightly elongated. There's a hint of minor disturbances in the galaxy shape, although it looks like it is not currently undergoing a major merger. Based on the data, the galaxy is of moderate apparent size, appearing unresolved in the image, yet not a point source. The color profile suggest the presence of an older stellar population in the galaxy.
