The galaxy appears as a centrally concentrated object, exhibiting a smooth, elliptical morphology. It is characterized by a bright, yellowish-white core that gradually fades into a diffuse outer region. The overall shape is close to round, showing only slight elongation. There is no apparent spiral structure, bar, or evidence of significant dust lanes. Nor are there visible signs of tidal disturbances or ongoing major mergers. The galaxy’s color profile indicates a likely population of older stars, potentially with minimal on-going star formation. The galaxy is relatively isolated, with no other visible galaxies nearby.
