The galaxy appears as an elliptical, or possibly lenticular, system exhibiting a smooth, diffuse light distribution with a noticeable central bulge. The color profile indicates a reddish hue across the galaxy, suggesting an older stellar population with a lower rate of current star formation. The system appears elongated with a relatively high axis ratio, indicating a deviation from a perfect spherical shape. There is no visible evidence of spiral arm structure, dust lanes, or tidal features indicative of recent or ongoing mergers or strong interactions with other galaxies. The lack of blue light suggests that the galaxy is primarily composed of older stars. The apparent size is small, indicative of substantial distance.
