The galaxy appears as a singular, relatively smooth object with an elliptical morphology. There is a concentration of light towards the center, suggesting a prominent bulge. No distinct spiral arm structures are apparent within the visible light wavelengths. The galaxy exhibits a reddish-yellow hue, indicating a population of older stars. There is no evidence of significant dust lanes or recent star formation regions from visual inspection, further supporting the inference of an older stellar population and a relatively quiescent state. The galaxy seems to be isolated with no signs of interactions or merging events. The galaxy displays a concentrated, symmetrical shape without obvious disturbances.
