The galaxy appears as a centrally concentrated object with a smooth morphology. There is little evidence of distinct spiral arms or a pronounced disk structure. The object's light profile suggests a bulge-dominated system, potentially an elliptical or S0 galaxy. The color gradient indicates a relatively old stellar population dominating the core, shifting toward slightly bluer colors in the outer regions. There are no obvious signs of ongoing major merging activity or strong tidal disturbances in the galaxy's immediate vicinity. The overall shape is somewhat elliptical, but closer to round, with only a slight elongation visible. Based on the light profile and smooth features, this galaxy likely represents a quiescent system with suppressed star formation within the core.
