The galaxy presents as a centrally concentrated, elliptical-like object with a smooth light distribution. Its core is bright and nearly circular, with a gradual decrease in luminosity moving outwards, exhibiting a slight elongation or cigar shape. There are faint, diffuse features extending from the main body, but no clear spiral arms or distinct structures are visible. The color appears to be a relatively uniform blue-white across the galaxy, suggesting a mixture of stellar populations with a likely predominance of older stars. There is no evidence of ongoing major mergers. The galaxy seems relatively undisturbed.
