The galaxy appears to be an elliptical type, exhibiting a generally smooth and rounded morphology. The light distribution suggests a centrally concentrated bulge, with a gradual decrease in luminosity towards the outer regions. There's a noticeable lack of distinct spiral arms or a prominent disk structure. The galaxy's color profile indicates a redder hue, consistent with an older stellar population and a lower rate of ongoing star formation. There's no obvious evidence of significant tidal disturbances or ongoing mergers, suggesting it's relatively undisturbed. Overall, the galaxy presents as a well-formed, evolved system.
