The galaxy presents as a relatively smooth, centrally concentrated object. Its overall morphology suggests an elliptical or lenticular classification, with minimal evidence of spiral arm structures. The light distribution appears centrally symmetric, and the shape is close to round. The core is bright, exhibiting a yellowish hue indicative of an older stellar population. This color may be due to redshift effects. Fainter, extended regions surround the central core and they become more red/brown further out. The overall light profile appears smooth and diffuse. There is no obvious sign of recent or ongoing major mergers, although some minor disturbances cannot be ruled out given the resolution. Overall star formation activity appears low.
