The galaxy appears to be an elliptical galaxy, characterized by a smooth, diffuse light distribution. The galaxy displays an overall orange-red hue, suggesting an older stellar population with a lower rate of active star formation. The central bulge region exhibits higher luminosity and a more pronounced orange-red color, indicative of a concentration of evolved stars. The isophotes appear mostly regular, with some hints of asymmetry in the outer regions, potentially due to minor tidal interactions or internal disturbances. The morphology suggests a lack of prominent spiral arms or a well-defined disk structure.
