The galaxy presents as a well-defined elliptical structure with a smooth, centrally concentrated luminosity profile. The central region exhibits a yellowish hue, suggesting a population of older stars. Moving outward from the core, the color gradually shifts toward a bluer tone, potentially indicating the presence of younger stellar populations or a degree of ongoing star formation. There is a noticeable elongation along one axis, with a cigar-like shape. No prominent spiral arms, dust lanes, or signs of recent major mergers are apparent. There are no clear visual signs of strong tidal interactions. Overall, the galaxy appears to be a relatively undisturbed, evolved system.
