The galaxy exhibits a generally elliptical morphology. A bright, concentrated core region is clearly visible, suggesting a significant stellar density at the galactic center, and there appears to be a smooth decline in surface brightness extending outwards from the core.

The galaxy's overall color profile indicates a redder hue. This suggests a population dominated by older stars and a relatively low rate of ongoing star formation. There is little evidence of prominent spiral arms or distinct dust lanes, supporting its classification as an elliptical galaxy. The image also shows that the galaxy may be a disk galaxy seen at an angle, where the roundness of the disk is somewhere in between a circle and a cigar shape. I don't see any major disturbances in the galaxy due to merging or other major interactions.
