The observed galaxy presents as a relatively compact object. It displays a diffuse, somewhat amorphous structure. There appears to be a slight irregularity in its morphology, but it is not highly pronounced. The galaxy exhibits a subtle, uneven brightness distribution across its body, hinting at possible substructure or uneven star formation. The object's color suggests a population of older stars. No clear spiral arms or disk are discernible, indicating that it is likely an elliptical or irregular galaxy type. The galaxy appears to be relatively isolated, with no obvious signs of strong tidal interactions with neighboring galaxies. There seems to be some minor disturbances to its morphology, but it is overall a fairly isolated system.
