The galaxy presents as a centrally concentrated, smooth object, suggestive of an elliptical morphology, with a slight elongation. A bright, relatively small core region dominates the galaxy's light output. The color profile indicates a reddish-orange central region, transitioning to a greenish-yellow hue in the outer regions. This color gradient may indicate varying stellar populations, with older, redder stars concentrated towards the center and slightly younger, bluer stars in the surrounding areas. No distinct spiral arms or prominent dust lanes are discernible, further supporting the elliptical classification. The galaxy appears relatively undisturbed, showing no signs of ongoing major mergers or significant tidal interactions. Some very faint asymmetry is noted at the edges of the light profile, but is difficult to resolve whether this is real, or due to noise. It has a moderate size based on the image scale, but due to unknown distance this can not be confirmed.