The galaxy presents as a moderately bright, relatively compact object with a somewhat smooth, elliptical morphology. Its core region exhibits a higher surface brightness and a yellowish hue, suggesting an older stellar population is dominant in this area. Extending outward from the central bulge, a fainter, bluer disk is visible. This implies ongoing star formation, although at a modest rate, in the outer regions. The disk does not show prominent spiral arm structures. Faint asymmetries may be present in the outer disk, potentially indicative of minor gravitational interactions or past merger events. Overall, the galaxy appears as a transition object between early-type and late-type galaxies, with characteristics of both elliptical and spiral morphologies.
