The galaxy appears to be a relatively smooth, centrally concentrated object, suggesting an elliptical or lenticular morphology. There is little evidence of spiral arms or prominent dust lanes. The galaxy exhibits a moderate degree of ellipticity, appearing somewhat elongated rather than perfectly spherical. The color profile is suggestive of an older stellar population, with a redder hue in the central regions, potentially indicative of a high concentration of evolved stars. A slight blue color in the outer regions may indicate a small amount of on-going star formation. There is no obvious evidence of strong tidal features or ongoing mergers, although minor disturbances cannot be ruled out. Overall, the galaxy appears to be a fairly isolated, evolved system.
