The galaxy appears to be a relatively compact elliptical galaxy, exhibiting a smooth, concentrated light profile. It appears almost spherical, with no discernible spiral arms or bar structures. The core region is bright, gradually fading into its outer regions. The galaxy exhibits a redder hue, which may be indicative of an older stellar population with lower rates of ongoing star formation. There is a slight hint of minor disturbance or asymmetry in its shape.
