The galaxy appears as a relatively smooth, elliptical structure. Its light is predominantly concentrated towards the center, with a gradual decrease in surface brightness towards the outer regions. There is a subtle elongation, suggesting it is not perfectly spherical, but rather somewhere between round and cigar-shaped. There is no clear evidence of distinct spiral arms or a prominent disk structure, and the galaxy shows little to no signs of major mergers or significant tidal disturbances. Based on its color profile and the presence of an apparent lack of intense star formation, this galaxy may be a relatively quiescent system, dominated by an older stellar population.
