This galaxy presents as an intermediate system, exhibiting characteristics of both elliptical and spiral morphologies. It displays a central, bright bulge that appears relatively smooth and concentrated. Surrounding the bulge, there is a fainter, more diffuse disk component, though distinct spiral arms are not clearly visible. The overall color suggests a galaxy with a mix of stellar populations, with the bulge likely dominated by older, redder stars and the disk exhibiting a bluer hue, potentially indicative of ongoing star formation. The galaxy appears to be slightly elongated, but largely without significant disturbances or tidal features, pointing toward a relatively settled state.
