This galaxy appears to be an elliptical galaxy at an estimated distance that corresponds to a redshift of approximately 0.065. The galaxy exhibits a smooth, centrally concentrated light profile, with the majority of the light emanating from the core. The shape of the galaxy is neither perfectly round, nor highly elongated. The color profile displays a general red-yellow hue, indicative of an older stellar population and suppressed star formation. There is no discernible spiral arm structure or significant dust lane features. No signs of a major ongoing merger or strong tidal disturbances are visually apparent. There appears to be a slight asymmetry, but its cause is unclear. Overall, this galaxy is consistent with a relatively quiescent elliptical system.
