The galaxy presents as a slightly elongated, relatively smooth structure with a prominent central bulge. The bulge exhibits a yellowish hue, suggesting an older stellar population. A faint, diffuse disk surrounds the bulge, displaying a bluish tinge indicative of ongoing or recent star formation. This disk appears moderately inclined relative to our line of sight.  There appears to be some distortion or irregularity in the outer regions of the disk. The galaxy exhibits an approximate size of 6.4 kpc, with an elliptical shape. There is some evidence of minor disturbances likely due to galactic merging.