The galaxy appears to be an elliptical galaxy, exhibiting a generally smooth and rounded morphology. There is minimal evidence of spiral arms or distinct features within the galaxy's structure. The light distribution is fairly uniform across the galactic body, suggesting an older stellar population and a lack of significant ongoing star formation. Some small disturbance can be seen, possibly a recent merger. The colour index suggests that the galaxy is redder than average, which is consistent with an older stellar population, with small evidence of bluer regions.
