The galaxy presents as a somewhat diffuse, centrally concentrated object. Its morphology is predominantly smooth, with a subtle elongation suggesting a possible flattened structure. The color profile exhibits a general trend where the central region appears slightly more blue-shifted than the outer regions. This may indicate ongoing star formation or the presence of a relatively younger stellar population within the galactic core. There is a slight asymmetry in the outer edges of the object, potentially hinting at minor gravitational interaction or disturbance. There is a clear absence of spiral arms or well-defined disk-like features, suggesting the galaxy is likely elliptical or lenticular. There also seems to be a slightly disturbed morphology. The relatively small angular size indicates that it is likely a distant object.
