The galaxy presents a largely smooth and elliptical morphology. It appears to be a concentrated spheroid of light, exhibiting a radial gradient where brightness decreases further from the center. A slight elongation is observed, suggesting a mild departure from perfect circular symmetry. There is no visible spiral arm structure or prominent dust lanes. The galaxy exhibits a yellow-red hue. There is some suggestion of minor disturbances, but the main body of the galaxy appears relatively undisturbed. The stellar population consists primarily of older, redder stars.
