The galaxy presents an overall ellipsoidal morphology with a moderate degree of internal structure. There is evidence of disruption, with some asymmetries visible in its shape and light distribution. The central region exhibits a yellowish hue, possibly indicative of an older stellar population, while the outer regions are characterized by a bluer tint, suggesting ongoing or recent star formation. There are some hints of tidal features and potentially minor disturbances, indicating possible interaction with another galaxy. The galaxy exhibits a fairly concentrated profile, with luminosity decreasing from a central peak.
