The galaxy presents a generally smooth and featureless appearance. It exhibits a roughly elliptical morphology, appearing somewhat rounded but not perfectly circular. The color profile suggests a dominant population of older stars, as indicated by the relatively redder hue. There is no clear evidence of spiral arms or a pronounced disk structure, indicating a likely classification as an elliptical galaxy. The galaxy does not appear to be undergoing any major merging events, although subtle asymmetries could indicate minor disturbances or interactions. The overall impression is of a relatively evolved system with a high degree of internal homogeneity.
