The galaxy presents a generally smooth morphology, with a dominant spheroidal component. Its shape appears roughly round, exhibiting minimal elongation. The light profile suggests a concentration towards the center. No prominent spiral arms or bar structures are discernible. The color is yellowish overall, hinting at an older stellar population with suppressed current star formation. There is some evidence of minor disturbances in the outer regions. The galaxy appears to be isolated, lacking close companions or signs of ongoing major mergers.
