The galaxy presents an overall smooth morphology, appearing as a relatively undisturbed system. The main body of the galaxy exhibits a concentrated central bulge that transitions into a slightly elongated structure. The light distribution suggests a moderate degree of central concentration. The galaxy exhibits a color gradient from the center outwards, with the central regions appearing more yellow/orange, suggestive of an older stellar population. Fainter, bluer regions are observed further from the center, which may indicate more recent star formation activity. There is an indication of a tidal tail, with the possibility of smaller objects in line with the galaxy, perhaps indicative of minor disturbances or possible merger activity. The system appears to be of intermediate size. The outer edges of the galaxy are diffuse and ill-defined, merging gradually into the background sky. The general shape is neither perfectly spherical nor a highly elongated cigar shape, falling somewhere in between. The system appears primarily quiescent, but with some evidence of minor star formation.
