The galaxy presents as a moderately luminous, yellowish-white elliptical morphology. The light distribution appears relatively smooth and centrally concentrated, with a slight elongation suggesting an oblate spheroid shape rather than a perfect sphere. There is no obvious indication of spiral arms, a bar, or significant dust lanes. The galaxy appears relatively isolated with no clear signs of ongoing major mergers or tidal disturbances. Its color suggests a population dominated by older stars, indicating a cessation of significant star formation in the recent past. There is a slight asymmetry in the galaxy, with a hint of fuzziness on one edge.
