The galaxy presents a generally smooth, elliptical morphology with a bright, concentrated central bulge. There is a subtle flattening, suggesting it may be classified somewhere between round and cigar-shaped, but it is primarily elliptical. A faint disk-like structure might be present but it lacks distinct spiral arms. There is little evidence of significant ongoing merging activity, although subtle disturbances in the outer regions cannot be ruled out. The galaxy exhibits a color gradient, appearing more yellowish in the central regions, suggestive of an older stellar population, transitioning to bluer hues in the outer regions, which is indicative of younger stars and ongoing, but still relatively low, star formation.
