The galaxy presents as a relatively smooth, elliptical morphology. Its light distribution appears centrally concentrated, with a radial falloff in intensity from the core. Color gradients are subtle, with the core region exhibiting a yellowish-white hue, potentially indicative of an older stellar population. The outer regions show a slight reddening compared to the core, although the image resolution limits detailed color analysis. No distinct spiral arms or significant dust lanes are visible, suggesting a lack of ongoing major star formation. The overall shape is approximately circular, with only minor deviations from perfect symmetry. There is no visual evidence of any major mergers or tidal disturbances. The galaxy appears to be relatively isolated.
