The galaxy presents as a moderately bright, elliptical morphology. The central bulge exhibits a strong concentration of light, appearing a yellowish-white hue, indicative of an older stellar population. Moving outwards from the core, the light intensity diminishes gradually. There appears to be a lack of distinct spiral arm structure. The galaxy exhibits a relatively smooth overall appearance, suggesting a lack of ongoing major star formation. The elongation of the galaxy suggests a non-spherical shape, tending towards a more flattened, disc-like structure despite its classification as elliptical. No significant tidal features or signs of recent major merger events are visible. Marginal disturbances may be present in the outer halo.
