The galaxy presents a largely smooth and rounded morphology. It appears to be an elliptical or lenticular galaxy, exhibiting a concentrated central bulge that gradually fades into the outer regions. There are no visible spiral arms or significant dust lanes; the overall structure is quite uniform, suggesting a lack of active star formation. The color profile indicates a dominance of older stellar populations, giving it a reddish hue. There is no indication of ongoing mergers or tidal disturbances. The galaxy appears undisturbed and in a relatively relaxed state.
