The galaxy presents a generally smooth, elliptical morphology. The central bulge is prominent and exhibits a concentrated, yellowish hue, suggesting an older stellar population. Moving outward from the core, the light gradually diffuses, with a slight elongation along one axis, giving it a somewhat cigar-like appearance. There is faint evidence of a possible disk, based on the slightly enhanced emission in a flattened plane compared to the poles. No obvious spiral arm structure or dust lanes are discernible within the image. There is a subtle color gradient from the core outwards, showing a shift towards slightly bluer colors in the outer regions, which could indicate the presence of some younger stars. There does not appear to be any significant merging activity or tidal disturbances. Overall, it is a galaxy with a smooth profile, likely an elliptical or lenticular galaxy at a redshift of approximately 0.2.
