The galaxy appears as a centrally concentrated, elliptical-like structure. It exhibits a generally smooth morphology with no obvious spiral arm features or distinct disk-like appearance. The light distribution is relatively uniform, fading gradually from the core outwards. There may be a slight elongation, making it not perfectly circular, however the shape is predominantly round with no noticeable distortions suggestive of a major merger event. The object shows little evidence of ongoing star formation activity, appearing quiescent. No pronounced dust lanes or regions of intense blue light are detected. There are no nearby galaxies in the immediate vicinity that would indicate a possible interaction or tidal disturbance. Overall, the galaxy presents a classic smooth and rounded appearance, consistent with an early-type or elliptical classification.
