The galaxy presents as a single, concentrated body of light, exhibiting a smooth, largely featureless morphology. Its overall shape appears roughly circular, with the light intensity gradually decreasing from the center outwards. There is a concentrated, bright central region. The color profile skews toward the red end of the spectrum, suggesting a stellar population dominated by older stars. There is no discernible spiral structure, bar, or dust lane. A slight asymmetry may be present, but the signal is weak.
