The galaxy presents as a largely homogenous, elliptical structure. It appears to have a high degree of central concentration, with luminosity decreasing gradually outwards from the core. The galaxy exhibits a smooth, rounded morphology. A slight elongation is discernible, but it is minimal. Its color profile suggests a population of older stars, as indicated by its redder hue, specifically in the R and Z bands, with lower emission in the G band. There is no strong evidence of prominent spiral arms or a distinct disk. Furthermore, there are no immediately obvious signs of recent or ongoing major mergers or tidal disturbances from external sources. There is some evidence of star formation but it appears to be largely quiescent at the moment.
