The galaxy presents as a relatively smooth and rounded structure. The light profile appears to be centrally concentrated with a gradual decrease in intensity moving outwards, indicative of a high Sersic Index, possibly greater than 4, suggesting a classical bulge morphology. There does not seem to be significant disc morphology. Its color is slightly red, indicative of an older stellar population. Its size appears compact. There is no obvious spiral structure or prominent dust lanes visible. There are no signs of any merging galaxies or any irregular morphology.
