The galaxy appears as a relatively smooth, centrally concentrated object with an elliptical morphology. There is a lack of discernible spiral arm structure or significant dust lanes. The light distribution suggests a bulge-dominated system. The galaxy exhibits a yellowish-orange color, indicative of an older stellar population with relatively low levels of ongoing star formation. The overall form is generally round, but with a hint of elongation. There are no signs of any major ongoing mergers or significant tidal disturbances. The galaxy appears relatively isolated.
