The galaxy presents an elongated, cigar-shaped morphology, indicating it may be an elliptical galaxy or a spiral galaxy viewed edge-on. It exhibits a smooth, diffuse light distribution, with a concentration of light towards its center. The color profile suggests an older stellar population, potentially dominated by redder stars, and a low rate of star formation. There is a possibility of minor disturbance or interaction given the slight asymmetry. Its estimated size suggests it is a relatively small galaxy.
