The galaxy presents a predominantly smooth morphology, with a somewhat elliptical shape. It exhibits a bright, concentrated central region, likely a galactic bulge. Fainter, diffuse extensions surround this core, indicating a possible disk component, although the image resolution does not allow for a conclusive assessment of spiral arm structures. The overall color appears slightly redder in the central region, transitioning to a bluer hue in the outer regions. This color gradient may be indicative of an older stellar population concentrated in the center and younger, hotter stars in the periphery, suggesting ongoing, but limited, star formation. There is no obvious evidence of major mergers or significant tidal disturbances in this image, although subtle distortions might be present upon further, higher-resolution analysis.
