The galaxy presents a generally smooth, elliptical morphology. There is a slight elongation, but it appears predominantly spheroidal. The central region exhibits a concentrated brightness, suggesting a prominent bulge. Color gradients indicate a redder hue toward the core, transitioning to slightly bluer tones in the outer regions. No distinct spiral arms or prominent dust lanes are visible, implying a lack of significant ongoing star formation. Overall, the galaxy appears to be a relatively evolved system with a population of older stars dominating its stellar content. There is no evidence of major mergers or significant tidal disturbances.
