The galaxy presents as a relatively smooth, elliptical structure. It exhibits a centrally concentrated luminosity profile, with brightness decreasing gradually outward from a bright, somewhat unresolved core. The overall shape is elongated, but not highly flattened. The color gradient suggests an older stellar population. The core exhibits a yellowish-white hue, gradually transitioning to a redder color in the outer regions. This redder color suggests older stars and a lack of ongoing star formation in the outskirts. There is no obvious evidence of spiral arms, dust lanes, or significant irregularities in its morphology. It appears to be a relatively isolated galaxy, not clearly interacting with any other significant companions.
