The galaxy presents a generally smooth, elliptical morphology with a concentrated central bulge. The light distribution appears consistent and lacks any obvious spiral arm structures or significant dust lanes. There is a slight elongation in the morphology, but overall, it appears relatively rounded. The color profile suggests a population dominated by older stars, as indicated by the yellowish-orange hue, with a less active rate of current star formation, although it's still present. Any evidence of recent or ongoing mergers appears minimal, with no pronounced tidal tails or asymmetric features readily visible. Overall, the galaxy appears to be a relatively isolated elliptical galaxy in a stable state.
