The galaxy presents a generally smooth morphology, lacking prominent spiral arms or a well-defined disk structure. The light distribution suggests an elliptical or lenticular classification. A bright, concentrated central bulge dominates the galaxy's luminosity, indicating a high stellar density in the core region. The overall color appears yellowish-red, suggestive of an older stellar population with reduced star formation. There is an absence of significant dust lanes or ongoing star-forming regions. The galaxy exhibits a round shape. There is no apparent evidence of tidal tails, distortions, or close companions to suggest a recent merger event.
