The galaxy presents as a luminous, elongated structure. It exhibits a relatively smooth, featureless morphology, with a noticeable central bulge. The galaxy's color profile suggests an older stellar population, given its redder hue. There may be a subtle dust lane or obscuration present near the center, but the overall smooth appearance dominates. The galaxy does not appear to be undergoing any major merging activity, although there is a hint of a minor disturbance in its structure. Its form deviates slightly from a perfect elliptical shape, presenting an intermediary shape between round and elongated.
