The galaxy presents as a relatively smooth, elliptical-like structure. It displays a concentrated central bulge that appears to be comprised of older stellar populations, indicated by its yellowish-orange hue. There is minimal evidence of spiral arm structures or significant dust lanes. The overall morphology suggests a galaxy in a relatively late stage of its evolutionary development, with diminished star formation activity. A slight elongation is observed, though the galaxy tends toward a more rounded shape. There appears to be some minor gravitational interaction evidenced by the slight distortion of the overall form. Given the absence of significant ongoing star formation, the galaxy is likely a relatively massive system, which could be anywhere from 10^10 to 10^11 solar masses.
