The galaxy presents as a relatively smooth, centrally concentrated object. The light profile indicates a dominant spheroidal component. The central region exhibits a yellowish hue, possibly indicative of an older stellar population. Fainter, bluer regions are asymmetrically distributed outside the central region, suggesting the possibility of recent or ongoing star formation in the outer parts of the galaxy. There is no clear evidence of spiral arms or a well-defined disk structure. The galaxy appears largely undisturbed, without strong indications of a recent major merger event, although there could be subtle signs of minor tidal disturbances or interactions in the surrounding faint structure. Its overall shape is neither perfectly spherical nor highly elongated, placing it somewhere in between.
