The galaxy presents as a relatively smooth, elliptical-like structure with a concentrated central bulge. There is an absence of prominent spiral arms or significant dust lanes, giving it a generally featureless appearance. The central region exhibits a yellowish hue, possibly indicative of an older stellar population. Fainter, bluer light extends outward from the core, potentially suggesting some ongoing, albeit subdued, star formation in the outer regions. The overall shape is generally round. There is no obvious evidence of tidal interactions or major mergers.
