The galaxy presents as a relatively smooth, centrally concentrated object with an elliptical morphology. A dominant, yellowish bulge occupies the central region, indicative of an older stellar population. The outer regions display a fainter, more diffuse disk-like structure, with hints of spiral arms. There appears to be some minor disturbances in the galaxy's shape, but no major mergers or tidal tails are readily apparent. The galaxy has a slight tilt relative to our line of sight. The color suggests ongoing star formation, but at a moderate rate. Overall, the galaxy exhibits characteristics of an intermediate-mass system with a mixed stellar population and a disk-like structure.
