The galaxy presents as a largely featureless, elliptical or lenticular structure. Its light profile appears smooth and centrally concentrated, with a gradual decline in luminosity towards the outer regions. There is a slight elongation suggesting it is not perfectly spherical, trending toward a cigar shape. The core region exhibits a yellowish-white hue, which likely indicates an older stellar population. There is little evidence of prominent spiral arms, dust lanes, or active star-forming regions, giving it a relatively passive appearance. There may be the beginning of a minor interaction or disturbance, but it does not look like a current or recent major merger.
