The galaxy presents a complex morphology, exhibiting characteristics that suggest both smooth, spheroid-like structures and features indicative of a disk. The central region displays a concentrated, yellowish hue, implying a significant population of older stars or substantial dust obscuration. Extending from the core is a fainter, bluer component, possibly representing a disk or spiral arms where active star formation is occurring.

There are irregularities and disruptions in the disk or outer regions of the galaxy, indicating potential gravitational interactions or ongoing mergers. The overall structure is not entirely smooth, showing some distortions that could arise from past or present tidal forces. The integrated light suggests moderate star formation activity.

Based on its color and structural features, this galaxy appears to be at an intermediate stage of evolution, possibly transitioning from a spiral-dominated to an elliptical-dominated system, with ongoing dynamic processes influencing its morphology.
