The galaxy exhibits a largely smooth morphology, with a notable absence of prominent spiral arms or a distinct disk structure. It presents a roughly elliptical shape, deviating only slightly from a perfect circle. The galaxy's core region is characterized by a bright, concentrated light, suggesting a high density of stars. The light from the core gradually diffuses outwards, forming a fainter, extended halo. The color profile indicates a redder hue, particularly prominent in the central regions, possibly indicative of an older stellar population. There is no visual evidence of significant tidal disturbances or ongoing major mergers, although subtle irregularities in the outer regions might suggest minor gravitational interactions or past mergers. Star formation appears to be relatively quiescent, with little to no discernible blue color indicative of young, massive stars.
