The galaxy presents as a primarily smooth, elliptical structure with a concentrated central bulge exhibiting a yellowish hue, suggesting an older stellar population. The light distribution appears relatively even across the galaxy, with a subtle decline in intensity moving from the core to the outer regions. There is some indication of faint, disk-like structure or faint features, however, there are no distinct spiral arms that can be identified. The shape is elongated, but appears close to round. There appears to be some possible indication of minor tidal disturbance or interaction on the galaxy's edge, but no evidence of major merging.
