The galaxy presents a largely smooth, elliptical morphology. There is a notable concentration of light towards the galactic center, suggesting a prominent bulge. The color profile appears relatively uniform, with a subtle gradient from a warmer, yellowish core to slightly cooler hues in the outer regions. The isophotes show a slight degree of ellipticity, deviating marginally from a perfectly circular shape. There is no clear evidence of spiral arm structures or significant dust lanes. Faint, diffuse extensions may be present, but are not clearly defined. The overall appearance suggests a system dominated by an older stellar population, and there is a possible indication of a minor interaction or disturbance.
