The galaxy appears as a diffuse, centrally concentrated object with a roughly elliptical morphology. Its color suggests the presence of a mix of stellar populations, with hints of younger, bluer stars intermixed with older, redder populations. There appears to be a smooth transition in light intensity from the core of the galaxy outwards, consistent with a relatively relaxed structure. While there isn't clear evidence of spiral arms or a prominent disk, a subtle, faint feature could be interpreted as a distorted disk component. The overall structure suggests an evolved system, possibly undergoing or having undergone a minor merger event, disrupting a previously established disk morphology. The outer regions of the galaxy gradually fade into the background, indicating the absence of a sharp edge or truncation.
