The galaxy presents as a singular, relatively smooth structure. Its overall form appears elliptical, trending towards a flattened spheroid, but without a pronounced disk. There may be a slight deviation from perfect roundness, but it is subtle. The galaxy exhibits a yellowish-red hue, suggesting an older stellar population and lower ongoing star formation. The smooth appearance indicates a lack of significant recent mergers or major disturbances. There is no obvious spiral structure or prominent dust lanes visible. Faint blue regions suggest a low level of ongoing star formation.
