The galaxy presents as a somewhat smooth, elliptical-like structure with a concentrated central bulge. There is an indication of a disk shape, oriented roughly horizontally across the image. The central region exhibits a significantly brighter, more compact appearance, suggesting a high stellar density or perhaps an active galactic nucleus, though further spectral analysis is needed to confirm AGN activity. 

The galaxy shows a general blue hue, particularly in the central region. There is a hint of redness in the outer edges. This suggests a population of young, hot stars contributing to the overall color. There is no obvious evidence of strong tidal features or major disturbances suggesting recent major merger activity, though there might be minor signs of interaction. The galaxy appears relatively isolated, contributing to a less disturbed morphology.
