The galaxy presents an overall smooth morphology, with a dominant central bulge that appears approximately round. The luminosity profile suggests a centrally concentrated light distribution. Faint, diffuse extensions are tentatively observed, perhaps indicating minor tidal interactions or past merger events. Color gradients are present, with the central region appearing more yellow-orange, possibly indicative of an older stellar population, whereas the outer regions show a slightly bluer tint, suggesting the presence of some younger stars. The galaxy shows a very slight disk-like structure. There may be a faint, ill-defined spiral arm structure, but it is not prominent. There is evidence of some disturbances, possibly indicative of past mergers, but there is no major merging.
