The galaxy presents as a moderately bright, centrally concentrated elliptical type. It exhibits a smooth, diffuse light profile, with a significant fraction of its light emanating from the central bulge. The galaxy appears somewhat elongated, but not highly so, with an intermediate axial ratio. There is no readily discernible evidence of spiral arm structures or significant dust lanes. The color is relatively uniform across the galaxy, appearing slightly bluer in the central region, suggesting a modest amount of recent star formation activity relative to the overall stellar population. There is only very slight evidence of any tidal disturbance or merging activity in its immediate vicinity. It appears to be a relatively undisturbed, mature galaxy.
