The galaxy presents as a relatively compact object with an overall smooth appearance. There is a centrally concentrated luminosity that decreases gradually towards the outer regions, giving the impression of an elliptical morphology. The color gradient is subtle; the central region is a warmer hue, transitioning to cooler tones towards the periphery.

A minor asymmetry is observed in the galaxy's shape and luminosity distribution, indicating a possible gravitational interaction. A faint plume or tidal feature extends from the main body of the galaxy, further suggesting a past or ongoing merger event. The galaxy lacks any clear spiral arm structures or prominent dust lanes.
