The galaxy appears to be a smooth, elliptical or lenticular type galaxy, exhibiting a centrally concentrated and diffuse morphology. There is no observable spiral arm structure or significant dust lane features. The galaxy's shape is mostly round with some slight elongation. The primary color is yellowish. This suggests a population of older stars dominates the light output. There is no obvious evidence of ongoing major mergers or tidal disturbances, although some minor interaction cannot be ruled out at this resolution. The galaxy exhibits a noticeable red-shift. Based on the color index, it is likely composed of an older stellar population. The overall appearance suggests a relatively evolved system.
