The galaxy presents a moderately smooth profile, exhibiting a concentrated central region that transitions gradually into a more diffuse outer halo. The overall shape appears to be elliptical, deviating slightly from a perfectly circular form. There is little evidence of distinct spiral arms or significant disk-like structures. Subtle asymmetries or minor distortions are present, hinting at possible past or ongoing gravitational interactions, though no major merger events are immediately apparent. The galaxy's color profile suggests a population of relatively older stars, with a discernible lack of bright, young, blue stars indicative of recent star formation. The central region appears somewhat brighter and potentially slightly redder than the outer regions.
