The galaxy presents as a relatively well-defined, although somewhat disturbed system. The central region exhibits a high degree of luminosity, appearing smooth and concentrated. A slight reddish hue is discernible in the core, possibly indicative of an older stellar population. Moving outward from the core, a diffuse, bluer halo is observed, suggesting the presence of younger, hotter stars and possibly some ongoing star formation. There is evidence of asymmetry in the outer regions, particularly on the left, which could suggest a minor interaction or recent merger event. Some slight distortion in the galaxy's overall shape can also be noted. It appears to be somewhere between a pure elliptical galaxy and a spiral galaxy.