This galaxy appears to be a relatively smooth, disk-dominated system with a prominent central bulge. The galaxy's light is concentrated in the central region, suggesting a high stellar density within the bulge. The galaxy has a slight ellipticity, appearing somewhat elongated rather than perfectly circular. A faint disk is observable surrounding the central bulge. This galaxy is likely a spiral galaxy that is oriented approximately edge-on with respect to our line of sight. No strong signs of ongoing mergers or significant tidal disturbances are evident, indicating a relatively quiescent state for this system. The overall color profile suggests a mix of stellar populations, with older, redder stars concentrated in the bulge and potentially younger, bluer stars populating the disk.
