The galaxy appears to be generally smooth in texture with an elliptical morphology. It exhibits a high degree of roundness. The light distribution suggests that the galaxy is centrally concentrated. There is faint red emission observed from this galaxy, indicating older stellar populations, but there also appears to be some blue emission present, albeit less significant, which may indicate recent star formation. No distinct spiral arms or bar structures are apparent. There is no strong evidence for any major ongoing mergers or significant tidal distortions from what can be determined through visual inspection. There may be minor disturbances present in the galaxy's outer regions.
