The galaxy appears as a relatively smooth, elliptical structure. Its central region exhibits a concentrated, yellowish-white luminosity, suggesting a higher density of older stars. The outer regions fade into a more diffuse, reddish halo. A slight asymmetry is observed, possibly indicating a minor gravitational interaction or internal disturbance, though there is no clearly visible merging activity. The galaxy presents a generally rounded morphology with a subtle elongation along one axis, but nothing that looks cigar-shaped. The colors suggest ongoing star formation, possibly concentrated in the central region, given the color profile. No distinct spiral arms or prominent dust lanes are visible at this resolution, reinforcing the impression of an elliptical galaxy.
