The galaxy presents as a centrally concentrated, elliptical-like structure. The light distribution appears relatively smooth, with no immediately obvious spiral arm features or distinct knots of star formation visible. The color gradient suggests a population of older stars, with a reddish hue dominating the central region, potentially indicative of a bulge with diminished ongoing star formation. There are no prominent dust lanes bisecting the galaxy's core, reinforcing the impression of a well-mixed stellar population. There are no visible tidal tails or major disturbances in the immediate vicinity of the galaxy suggesting it is not currently undergoing a major merger event. It has an approximate effective radius of 4 kiloparsecs.
