The galaxy presents a predominantly smooth morphology, with a slight elongation indicative of an elliptical or lenticular classification. The central bulge appears bright and concentrated, gradually fading into the outer regions. There are no distinct spiral arms or bar structures visible. The galaxy exhibits a yellowish-white hue in the central regions, suggesting an older stellar population, while the outer regions appear somewhat bluer, indicating the presence of younger stars or ongoing star formation. There is no clear evidence of significant dust lanes or tidal features, and the galaxy appears to be relatively undisturbed.
