The galaxy appears to be an elliptical galaxy, potentially of type E4-E6, exhibiting an elongated shape without a clear spiral arm structure. The galaxy has a smooth appearance, lacking in distinct features. There is a notable color gradient, with a yellowish central bulge, indicating a higher concentration of older stars. The outskirts appear slightly bluer, suggesting ongoing star formation, albeit at a lower rate than what is seen in typical spiral galaxies. The stellar mass is relatively high. There is a potential minor disturbance or interaction occurring in the galaxy, which does not indicate a major merger.
