The galaxy presents as a relatively smooth, elliptical morphology. It exhibits a concentrated central bulge with a bright, yellowish hue, likely indicating an older stellar population. The outer regions of the galaxy appear less defined, with a gradual fading in intensity. There is a slight elongation observed, deviating from a perfectly circular shape. A subtle reddish tint is visible in the halo surrounding the central bulge, suggesting the presence of some dust or a population of older, redder stars. No distinct spiral arm structures or significant dust lanes are discernible in this image. The overall appearance suggests a galaxy that is relatively evolved and quiescent in terms of star formation. There is no obvious evidence of any major interaction or merging events.
