The galaxy presents as a relatively smooth, disk-like structure observed at an oblique angle. The central bulge region exhibits a concentrated luminosity, appearing yellowish-orange in color, potentially indicating an older stellar population with lower rates of star formation. Extending outward from the bulge, a fainter, more diffuse disk is observed. This disk displays a subtle color gradient, shifting towards slightly bluer hues at the outer edges, suggesting the presence of younger, hotter stars possibly associated with ongoing or recent star formation activity. The overall morphology suggests a quiescent system without evidence of significant mergers or tidal disturbances, and based on the lack of distinct spiral arms, may be more similar to a lenticular or early-type spiral galaxy.
