The galaxy appears as a somewhat elliptical, centrally concentrated object. The core exhibits a bright, yellowish-white hue, suggesting a population of older stars. The outer regions display a slightly bluer tint, which might indicate more recent star formation activity, although the overall color distribution remains relatively homogeneous. There is no clear evidence of spiral arm structures or significant dust lanes within the resolution afforded by the image. The galaxy's morphology is generally smooth, showing no obvious signs of major disturbances such as tidal tails or merging events. There is a slight elongation suggesting it is in between round and cigar shaped, and that the object may be a lenticular galaxy, lying somewhere on the continuum between an elliptical and spiral galaxy. There's a slight possibility of minor interaction with another object although nothing conclusive can be said with current image resolution.
