The galaxy appears as a relatively smooth, centrally concentrated object, possibly elliptical or lenticular in morphology. The light distribution suggests a spheroidal component dominates, with a lack of distinct spiral arm structures or prominent dust lanes. There is a slight elongation in shape, transitioning between round and cigar-shaped, hinting at a mild asymmetry or a possible interaction, though no major disturbances are immediately visible. Its color is predominantly yellowish, indicative of an older stellar population and relatively low ongoing star formation activity.
