The galaxy presents a generally smooth morphology, with a dominant, centrally concentrated bulge. The light distribution is relatively uniform, showing a high degree of symmetry and a lack of prominent spiral arm structures or irregular features. The shape appears approximately round, transitioning subtly to a more elliptical form in the outer regions. There is a suggestion of a faint, diffuse disk component extending beyond the bright central region, though details are difficult to resolve. No strong evidence of ongoing major mergers or tidal disturbances is apparent. The galaxy exhibits colors indicative of a relatively evolved stellar population, with a significant fraction of older stars. There is a noticeable color gradient, with the core exhibiting slightly bluer hues compared to the surrounding regions, possibly indicating a low level of ongoing star formation activity within the central area.
