This galaxy exhibits a morphology suggestive of an early-type system. The galaxy presents as a centrally concentrated object with a smooth, diffuse appearance. The core region is characterized by a bright, yellowish-white luminosity profile, indicating a likely population of older stars dominating the stellar content. This central region fades outward, and the outer regions of the galaxy appear to extend with a less concentrated and more irregular shape. There is a possible faint indication of a flattened disk or a surrounding halo, but overall, it seems to be mostly a spheroidal component. This disk area appears to be dusty, and there is little evidence of significant ongoing star formation. There do not seem to be signs of recent major merger events.
