The galaxy presents a relatively smooth, elliptical morphology with a concentrated central bulge. The color index suggests a population of older stars, imparting a yellowish hue. The galaxy appears well-defined, showing minimal evidence of significant disturbances or active merging events. There is a lack of readily apparent spiral arm structure or significant dust lanes. The overall structure indicates that this is an evolved galaxy with a likely low star formation rate. It exhibits a somewhat rounded shape, tending more toward a circular appearance rather than a highly elongated form.
