The galaxy presents as a somewhat elongated, cigar-shaped structure with a smooth, diffuse appearance. The central region exhibits a brighter, more concentrated light profile, suggesting a higher density of stars. Moving outward from the center, the light gradually fades. There is a subtle color gradient observed; the central bulge appears slightly more blue, possibly indicating a higher population of younger, hotter stars, while the outer regions seem redder, potentially due to older stellar populations or dust obscuration. No distinct spiral arms or other fine structures are clearly visible. The overall form suggests that this is likely an elliptical galaxy. There is no clear evidence of any major ongoing merger activity or significant tidal disturbances. The galaxy appears relatively isolated, with no nearby bright companions visible in the immediate vicinity.
