The galaxy appears as a moderately luminous object with a slightly elongated, elliptical morphology. The galaxy's light is dominated by yellow and white hues, suggestive of an older stellar population. The overall structure appears relatively smooth, indicating a lack of prominent spiral arms or significant dust lanes. There may be a faint hint of a disk-like structure, but it isn't well-defined. A potential minor disturbance is detected in the structure of the object. The object does not appear to be undergoing a major merger. The central region is brighter and more compact than the outer regions, indicative of a higher stellar density.
