The galaxy presents as a relatively smooth, centrally concentrated object. Its overall form is elliptical, appearing mostly round in projection. There is evidence of a disk component within the galaxy, which is suggested by a subtle flattening along its periphery. The central region exhibits a bright, yellowish core, likely indicative of an older stellar population. Surrounding the core is a fainter, bluer halo, which is suggestive of more recent, ongoing star formation. The galaxy does not appear to be undergoing any major mergers or strong tidal interactions, however, there is a slight asymmetry or minor disturbance present.