The galaxy appears as a centrally concentrated, elliptical or lenticular-like object. It presents with a smooth, relatively featureless morphology. A clear spheroidal component dominates the light profile, and the concentration of luminosity increases towards the core of the galaxy. There is a slight elongation, and it has a fairly round appearance. The galaxy exhibits a yellowish hue in the central region, which may be indicative of an older stellar population. There are no obvious signs of spiral arms, a bar structure, or significant dust lanes. No strong tidal features or asymmetries are immediately apparent, suggesting that there are no major mergers or strong gravitational interactions occurring. The galaxy's overall appearance is consistent with that of a relatively quiescent system, with lower levels of on-going star formation.
