The galaxy presents as a centrally concentrated, largely homogenous spheroid of light. Its morphology appears smooth, with no discernible spiral arms or distinct features like dust lanes. The color is notably redder, suggesting a population dominated by older stars. The galaxy appears relatively isolated. Its shape is mostly round. The central concentration exhibits a more intense yellow hue, potentially indicative of a denser population of stars or a weak active galactic nucleus. There appears to be a nearby dwarf galaxy that shows some signs of tidal disruption.