This galaxy presents as a relatively compact, elliptical structure with a prominent, luminous core. The overall color index suggests a population dominated by older, redder stars. The galaxy appears largely smooth, with only a slight deviation from perfect ellipticity indicating some potential tidal disturbance or recent minor merger. The spatial extent of the galaxy, as estimated by its half-light radius, suggests a substantial physical size. Despite the presence of a red stellar population, there is no evidence of significant ongoing star formation. The observed morphology is consistent with a post-starburst or quiescent galaxy, likely on the red sequence. There is no visual indication of strong tidal tails or other signs of ongoing major merger activity. However, the slight asymmetry hints at past interactions. Overall, the object appears to be a relatively massive galaxy with suppressed star formation and morphological features indicative of a quiet evolutionary state.
