The observed galaxy appears as a centrally concentrated object with a generally smooth morphology. The core exhibits a bright, diffuse glow that fades gradually outward. The overall shape is roughly elliptical, appearing more rounded than elongated.

There is some subtle structure that may indicate a minor disturbance. Faint extensions or asymmetries can be seen in the outer regions. There may be some early stages of merging with another small galaxy, or the disturbances may be due to internal processes.

Coloration is primarily yellow-red, suggesting an older stellar population with few young, blue stars and a significant amount of dust. There is little to no evidence of spiral arm structure.
