This galaxy presents as a generally smooth, centrally concentrated system. The overall morphology appears to be elliptical, exhibiting a moderate degree of ellipticity. The central region displays a bright, yellowish hue, suggesting a population of older stars. Fainter, bluer regions extend outwards from the core, possibly indicating areas of more recent, albeit low, star formation. There is no strong evidence of spiral arm structure or a prominent disk. The galaxy does not appear to be strongly interacting or undergoing a major merger, though there may be minor disturbances in its outer regions.
