The galaxy appears to be an elliptical galaxy, exhibiting a smooth, centrally concentrated light profile. The object appears yellowish, suggesting a population dominated by older stars and a relatively low rate of ongoing star formation. There is no discernible spiral arm structure or dust lane evident in this image, supporting its classification as an elliptical. The galaxy appears somewhat diffuse, with no sharp boundaries observed. There is no distinct nucleus, but the central region is brighter than the outer regions. There may be a slight asymmetry, which could indicate a past or ongoing minor interaction with another galaxy. It does not appear to be undergoing a major merger, based on its morphology. The galaxy is relatively compact, subtending a small angular size. The smooth profile indicates a relatively old and relaxed stellar population.
