The galaxy presents an elliptical morphology, appearing elongated with a smooth, diffuse light distribution. The central region is noticeably brighter and more concentrated, suggesting a substantial bulge component. Faint blue hues extend from the core, potentially indicating regions of recent star formation. There is evidence of possible tidal disturbances or minor merging activity, based on asymmetries in the outer regions. Overall, the galaxy exhibits characteristics of a moderately massive system, with indications of ongoing or recent evolutionary processes.
