The galaxy presents a flattened, elongated morphology, indicating a possible disk-like structure viewed edge-on. The central region exhibits a concentrated luminosity, likely corresponding to the galactic bulge. A subtle color gradient is observable, transitioning from a bluer hue at the outer edges towards a redder tone in the central bulge. This suggests ongoing or recent star formation in the disk regions, with a potentially older stellar population dominating the bulge. The overall smooth appearance implies a relatively undisturbed structure, with no obvious signs of major mergers or significant tidal interactions. There appears to be some evidence of dust lanes within the galaxy's disk. The galaxy has a estimated stellar mass of approximately 10^10 solar masses. The star formation rate is relatively low, with a specific star formation rate suggesting a quiescent galaxy.