The galaxy presents as a concentrated central bulge surrounded by a relatively smooth, extended disk. The disk exhibits a subtle blue tint, indicating regions of ongoing star formation. There are no distinct spiral arms visible. The overall color profile leans towards the redder end, particularly in the central bulge, suggesting an older stellar population and a relatively quiescent star formation history. The shape of the galaxy appears somewhat elliptical but nearly round, but with a more noticeable red-yellow hue in the galactic center. There is no obvious evidence of tidal distortions or mergers, but some faint disturbance or interaction with a close companion cannot be ruled out. 
