The galaxy presents a generally smooth, elliptical morphology. It exhibits a concentrated central bulge, with light intensity decreasing gradually towards the outer edges. There is a slight elongation, but the overall form is largely spheroidal. The color profile suggests a dominant population of older stars, giving it a yellowish hue. No distinct spiral arm structures or prominent dust lanes are apparent. There is no evidence of major mergers or significant tidal distortions in the immediate vicinity.
