The galaxy appears as a relatively smooth, centrally concentrated object, exhibiting a primarily elliptical morphology. There is minimal evidence of spiral arm structure or significant dust lanes. The color profile is dominated by reddish-yellow hues, suggesting a population of older stars. The galaxy's light distribution appears largely uniform, with a high degree of rotational symmetry. There is no indication of any active galactic nuclei or other notable forms of nuclear activity. Given the apparent lack of significant disturbances, it's likely this galaxy has not experienced a major merger event recently. The compact size and relatively smooth structure suggest that it could be a compact elliptical galaxy.