This galaxy appears to be an elliptical type, characterized by a smooth, featureless morphology. There is no discernible spiral arm structure or dust lane present. The galaxy exhibits a centrally concentrated bulge that is slightly elongated. The galaxy's light distribution appears relatively homogenous, indicating a lack of significant star formation regions that would otherwise appear as bright knots of blue emission. It possesses a yellowish-white hue within the central region, which transitions to a bluer color at its outer regions. This may indicate older stellar populations dominating the core, with ongoing star formation in the outer regions. There is evidence of minor disturbance in the outer parts of the galaxy, but no major mergers or tidal tails can be seen. It exhibits characteristics of being relatively massive.
