The galaxy presents as an elliptical structure, exhibiting a smooth, concentrated morphology. The central region displays a bright, yellowish hue, indicative of an older stellar population. The intensity gradually decreases towards the outer edges. The overall shape appears somewhat elongated, but not highly distorted. There is no readily apparent disk structure or spiral arm features. No strong evidence of ongoing merging activity or major disturbances is observed in the galaxy's overall form, though subtle irregularities may be present upon closer examination. The color suggests this galaxy could potentially be on the red sequence.
