The galaxy presents as a relatively smooth, elliptical-like structure, with a prominent central bulge exhibiting a yellowish hue. There is little indication of well-defined spiral arms or significant dust lanes. The light distribution gradually decreases from the core outwards, suggesting a centrally concentrated stellar population. The shape is somewhat elongated, but more closely approximates an ellipse than a highly flattened disk. There appears to be a general lack of strong star-forming regions, based on the subtle colourations. There is no indication of a major ongoing merger event or significant tidal disturbances. The light is more concentrated in the central region and fades gradually towards the outer edges.
