This galaxy exhibits a generally smooth morphology, appearing elliptical in shape with a high degree of elongation. The color gradient suggests a concentration of older stellar populations toward the galactic center, exhibiting a reddish-orange hue. Moving outward from the center, a subtle color shift toward bluish tones is observed, which could be indicative of younger, hotter stars in the outer regions, though their contribution is minimal. There is no clear evidence of spiral arm structure or significant dust lanes. The galaxy lacks apparent signs of active galactic nuclei or recent major mergers, although a very faint asymmetry could suggest minor tidal interactions. Overall, it appears to be a relatively quiescent system undergoing moderate levels of star formation.
