The galaxy presents as a bright, centrally concentrated object. Its overall morphology appears elliptical, exhibiting a smooth light distribution with no obvious spiral arm structure. The galaxy's core region displays significant luminosity, suggesting a high density of stars and possibly the presence of an active galactic nucleus. A faint halo of diffuse light extends outwards from the core, gradually fading into the background. The galaxy exhibits a slightly elongated shape. There's a suggestion of minor disturbances or asymmetries, but this requires further investigation for confirmation. The color profile indicates a primarily redder hue, with a slightly blue tinge. There are no clear signs of ongoing major mergers.
