The galaxy presents as a relatively small, slightly elongated or disk-like object. A central, bright nucleus is apparent, surrounded by a more diffuse, fainter halo. There is an indication of some structure or asymmetry within the disk, but it is not strongly defined. A very small, disturbed feature can be seen near one edge of the halo, which could be indicative of minor disturbances in the galaxy. The overall color appears to be bluish-white, suggesting the presence of a younger stellar population and/or active star formation. However, the presence of a faint redder hue in the halo suggests some older stars could also be present. There is a possibility that the galaxy is undergoing a minor merger event, but further spectral analysis would be needed to confirm this hypothesis.
