The observed galaxy presents as a relatively small, elongated structure with a high degree of apparent smoothness. There is a suggestion of faint, extended arms emanating from the central region, but these features are subtle. The object's light appears to be predominantly concentrated in a central bulge, with a gradual decrease in luminosity towards the outer regions. There may be minor disturbances or irregularities in the galaxy's overall shape, possibly indicative of past or ongoing interaction with another celestial body. However, these potential disturbances are not prominent, and the galaxy's overall morphology is relatively undisturbed. The object does not appear to be undergoing a major merger, but there could be some minor interaction occuring.
