The galaxy presents as a somewhat amorphous structure, potentially an elliptical galaxy, or possibly a disk galaxy viewed at an oblique angle. There appears to be a relatively bright central bulge, exhibiting a yellow-ish color. A fainter, more diffuse halo surrounds this central region, extending along what seems to be a primary axis. This halo has a bluer hue, suggesting the presence of a younger stellar population, or a higher rate of on-going star formation.

There is a hint of possible tidal disturbances or asymmetries in the outer regions of the halo, indicating a past or ongoing interaction with another galaxy. Alternatively, these features may point to internal dynamic processes, such as a recent merger. The galaxy does not appear to be highly structured with well-defined spiral arms, suggesting a smoother, more homogenous stellar distribution.
