The galaxy presents a generally elliptical morphology with hints of spiral structure. The central bulge exhibits a yellowish hue, likely indicating an older stellar population. A fainter, bluer disk surrounds the bulge, suggesting ongoing star formation, albeit at a moderate rate. There appears to be some disruption in the outer regions, possibly indicating a minor merger event or tidal interactions. Overall, the galaxy appears to be a transition object, showing characteristics of both elliptical and spiral galaxies.
