The galaxy presents as a relatively smooth, centrally concentrated object. Its overall shape appears close to circular, with a slight elongation potentially indicating a flattened spheroidal structure. The central region exhibits a brighter, more intense luminosity, suggesting a higher stellar density or the presence of an active galactic nucleus. A faint, diffuse halo surrounds the central bulge, gradually fading into the background sky. The color profile suggests a dominant population of older stars, evidenced by the redder hue in the central region and the halo. There is minimal evidence of prominent spiral arms or significant dust lanes, implying a morphological classification towards the elliptical or lenticular galaxy types. Possible minor disturbances could be present in the outer regions, but the resolution is not sufficient to confirm this.
