The galaxy presents as a relatively smooth, centrally concentrated elliptical galaxy, roughly spherical in shape. The core exhibits a yellowish hue, suggestive of an older stellar population. There is a gradual decrease in luminosity from the core outwards, transitioning to a fainter, bluer outer halo, with no distinct spiral arm structures or prominent dust lanes visible. The overall morphology implies a lack of significant ongoing star formation. Subtle irregularities in the outer regions may indicate minor past interactions.
