The galaxy presents a generally smooth morphology, with a high degree of central concentration. Its shape appears largely elliptical, trending toward round. There is a noticeable color gradient, with a yellow-white core that fades outward into a reddish halo. This suggests an older stellar population dominating the core. There is no evidence of spiral arms or significant dust lanes. I do not detect any major merger activity, or large tidal tails, although minor disturbances are possible due to the slight irregularities in the outer regions of the halo. The galaxy's moderate redshift indicates that it is relatively distant. It would appear to be a relatively massive galaxy.
