This galaxy appears to be a relatively smooth object, with a generally elliptical morphology. There is a slight elongation along one axis, but it is not strongly cigar-shaped. The galaxy exhibits a color gradient, appearing slightly bluer in the central regions and becoming redder towards the outer edges. This could indicate ongoing or recent star formation within the galactic core, with older stellar populations dominating the periphery. There is little indication of strong spiral arm structures or significant dust lanes. Based on the relatively uniform light distribution, the galaxy likely underwent only minor disturbances in its recent history.
