The galaxy presents an overall smooth morphology, appearing as a concentrated, elliptical structure. The light distribution suggests a prominent bulge, characterized by a yellowish hue that becomes more intense towards the center. The galaxy exhibits a moderate degree of elongation, appearing somewhat cigar-shaped rather than perfectly spherical. There is no clear indication of spiral arms or a distinct disk-like structure. The overall color suggests a stellar population dominated by older stars. Subtle irregularities or minor disturbances may be present in the outer regions, though they are not immediately obvious. The system doesn't appear to be undergoing a major merger event.
