The galaxy appears as a relatively smooth, elliptical or lenticular structure, with a dominant central bulge. Its morphology suggests a system without significant spiral arms or prominent disk features. The galaxy exhibits a yellowish hue, which implies a stellar population dominated by older, redder stars, indicating it is likely to be a more evolved system with a substantial mass and moderate star formation rate. There is a suggestion of a faint, extended halo surrounding the main body. The shape is not perfectly circular, appearing slightly elongated, falling somewhere between round and cigar-shaped. Evidentially, the object does not exhibit any major signs of ongoing merger events or major disturbances. There is some minor asymmetrical feature in the halo structure.
