This galaxy exhibits a generally smooth morphology, yet displays clear signs of significant disturbance. The central bulge is prominent and somewhat rounded, appearing as a concentrated region of light. A faint disk is discernible, extending outwards from the bulge, but it lacks well-defined spiral arms. The overall color suggests a population of older stars, with a hint of blue suggesting recent star formation activity.

The galaxy appears to be undergoing a major interaction, evident in the asymmetries and distortions observed in its structure. This interaction is likely the cause of the disturbed morphology, triggering significant star formation. The presence of tidal features is hinted at, though indistinct due to image resolution.
