The galaxy presents as a largely homogenous, elliptical-appearing object. It exhibits a concentrated central bulge that appears slightly elongated. The color profile suggests a population of older stars dominating the light output, trending toward the redder end of the spectrum. There is a slight gradient in color outward from the center, but the change is subtle. No distinct spiral arms or bars are discernible. There's no clear evidence of active star formation regions or significant dust lanes, suggesting a relatively quiescent galaxy state. The overall morphology leans towards a spheroid shape.
