The galaxy exhibits a generally elliptical morphology with a smooth, concentrated central bulge. There is a subtle disk-like component surrounding the bulge. The galaxy appears to be moderately inclined relative to our line of sight. The central bulge is the brightest and most luminous region, with a slightly yellow hue. The outer regions of the disk component appear fainter, and show some faint blueish tones suggesting younger star formation. There is a slight asymmetry in the light distribution of the outer regions. This suggests a possible minor gravitational disturbance or interaction. Overall, it appears to be a relatively massive galaxy.
