The galaxy appears as a relatively small, faint, and somewhat diffuse object. Its overall morphology seems elliptical or spheroidal, lacking any prominent spiral arm structure. The light distribution is centrally concentrated, with a gradual decrease in brightness towards the outer regions. Color gradients are subtle, but the central region appears slightly redder than the outer parts, suggesting an older stellar population in the core. There might be some minor disturbance to its shape, indicating a possible past interaction or ongoing minor merger. Star formation activity appears to be low, as indicated by the faintness and redder colors. The galaxy is mostly in between a disk and spherical shape.
