The galaxy presents as a centrally concentrated, relatively smooth object. The light distribution appears elliptical, trending towards a circular shape. The core is bright, indicating a significant concentration of stars. There is an absence of prominent spiral arm structures or well-defined dust lanes.  A faint, extended halo of diffuse light surrounds the central region, gradually fading into the background. Some subtle irregularities are visible in the outer regions, hinting at possible minor disturbances. The overall color appears relatively uniform with a slight reddening towards the central bulge, which may suggest an older stellar population. The low rate of star formation is consistent with its redder color. There are no obvious signs of a major ongoing merger, although some minor tidal features could potentially be present.
