This galaxy appears to be a relatively smooth, elliptical or lenticular system. The light profile shows a centrally concentrated bulge region that decreases in intensity outwards, with only a suggestion of a disk structure. The galaxy is more elongated than circular, with a moderate ellipticity, tending towards an "in between" shape rather than perfectly round or cigar-shaped. There does not appear to be any significant tidal distortion or evidence of recent or ongoing major mergers. There may be a slight disturbance visible, possibly indicating a minor interaction or internal dynamics affecting the galactic structure. The galaxy displays a range of colors, with the central region appearing bluer than the outer areas. This suggests a gradient in stellar populations, where younger, hotter stars are more concentrated within the bulge region, and older, redder stars are located towards the edges. Star formation is potentially present, but not at high levels.