The galaxy presents as a relatively smooth, elliptical-like structure, with a noticeable lack of distinct spiral arms or a prominent disk. The color profile suggests a dominant population of older stars, indicated by the reddish hue in the galactic bulge and outskirts. There appears to be a small, bluer region in its center. The overall light distribution is relatively uniform, without pronounced knots or regions of intense star formation. There is a minor visual disturbance in the form of an irregularity or slight asymmetry in its shape, potentially indicative of a past or ongoing interaction with a smaller galactic structure. The galaxy does not appear to be undergoing a major merger event.
