The galaxy appears to be an elliptical or lenticular type, exhibiting a generally smooth and featureless morphology. The central bulge is prominent and exhibits a yellowish hue, suggesting an older stellar population dominating the core. Moving outwards from the center, the light profile decreases smoothly and gradually blends with the surrounding background. There is little to no evidence of spiral arms, dust lanes, or distinct star-forming regions within the visible structure. The overall shape is moderately elliptical, appearing neither perfectly spherical nor highly elongated. There appears to be little evidence of tidal disturbances, major mergers, or significant interactions with neighboring galaxies.
