The galaxy appears to be a relatively luminous object, exhibiting a morphology that is neither purely elliptical nor a well-defined spiral. There is a central, bright bulge that dominates the structure, suggesting a significant concentration of stars in this region. The bulge exhibits a yellowish-white color, potentially indicating an older stellar population.

Extending outwards from the bulge, a fainter, more diffuse disk-like structure is observed. Hints of spiral arms can be discerned, though they are not sharply defined. These regions appear bluer in color compared to the bulge, possibly indicative of ongoing star formation.

The overall shape is somewhere between round and elongated, appearing slightly cigar-shaped, without any signs of major ongoing mergers, though minor disturbances and interactions might have taken place in its past. The galaxy appears to be relatively isolated in its environment.
