The galaxy presents as a centrally concentrated object with a relatively smooth and diffuse morphology. There is no apparent spiral structure or distinct disk component. The central region appears brighter and more condensed, gradually fading into the outer regions. Its overall shape is somewhat elliptical, exhibiting a moderate degree of elongation rather than appearing perfectly circular. There are faint hints of possible irregularities or minor disturbances in the outer halo, though no prominent merging features or tidal tails are discernible. The color appears generally yellow-reddish. This observed morphology indicates a galaxy dominated by an older stellar population with minimal ongoing star formation.
