The galaxy presents a generally smooth, elliptical morphology, appearing nearly circular. The central region exhibits a bright, concentrated core, gradually fading into a more diffuse halo. Color gradients suggest some variation in stellar populations or dust distribution, with a central yellowish-red core, potentially indicating older stellar populations. The outer regions show hints of bluer colors, suggesting the presence of younger stars, although star formation activity appears to be relatively low. No distinct spiral arms or significant dust lanes are apparent, further supporting an elliptical classification. The galaxy appears relatively undisturbed, without signs of major mergers or tidal interactions.
