The galaxy presents as a single, fairly well-defined object with a concentrated central region. The overall morphology appears to be smooth and somewhat elliptical, though not perfectly round. A very slight elongation is visible. The galaxy appears to lack spiral arms or any other distinct features typically associated with disk galaxies. 

The color profile is largely consistent throughout, with a somewhat reddish/yellow hue, suggesting a population of older stars and a relative lack of recent star formation. There does not appear to be any significant dust obscuration visible. Overall, the galaxy appears to be relatively undisturbed, showing no obvious signs of major interaction or merging events, though some minor disturbances cannot be ruled out based on the image alone.
