The galaxy presents as a relatively smooth, elongated structure. Its overall shape is elliptical, with a notable central bulge that appears brighter and more concentrated than the surrounding regions. The color profile suggests a higher concentration of older stellar populations, particularly within the central bulge, exhibiting a yellowish-orange hue. Fainter, bluer regions extending from the central area hint at the presence of younger stars and potential ongoing star formation, albeit at a modest rate. There is no clear evidence of spiral arm structures or significant dust lanes. Subtle irregularities in the outer regions imply minor gravitational interactions or past mergers that have yet to fully homogenize into the overall smooth morphology. The galaxy is moderately massive, within the range typically associated with elliptical galaxies.
