The galaxy presents a largely featureless, elliptical morphology. Its light profile exhibits high central concentration, with a bright, luminous core that diminishes gradually towards the outer edges. The dominant color is a yellow-orange hue, suggestive of an older stellar population. No distinct spiral arms, dust lanes, or other disk-like features are discernible within the observed wavelengths, reinforcing the classification of the galaxy as elliptical. The overall roundness is very high. There is no evidence of any major mergers or tidal disturbances. The size appears moderately compact.
