This galaxy presents as an elliptical morphology, appearing largely smooth and spheroidal in shape. A central, luminous core dominates the galaxy's structure, indicating a high concentration of stars in this region. Moving outward from the core, the light gradually fades, suggesting a decreasing stellar density. The galaxy exhibits a noticeable elongation or oblateness, with the ratio of its major to minor axis indicating it is not perfectly spherical, possibly an E3-E5 on the Hubble scale. There is a subtle color gradient visible, transitioning from a yellower, redder hue in the central bulge to slightly bluer tones in the outer regions, suggestive of some ongoing, but perhaps weak, star formation activity at the edges. No distinct spiral arm structures or prominent dust lanes are discernible within the galaxy's disk. There is no apparent indication of any recent or ongoing major merger events, though subtle signs of minor tidal disturbances cannot be ruled out. The object is likely a massive system.