The galaxy presents an approximately elliptical morphology, though with subtle irregularities in its outer isophotes. Its light profile appears relatively smooth, suggesting a lack of prominent spiral arms or strong dust lanes. The central region exhibits a higher concentration of luminosity, possibly indicative of a galactic bulge or active galactic nucleus. There is evidence of some tidal disturbances or faint plumes extending from the main body of the galaxy, particularly in the lower region, possibly indicative of a minor merger event or gravitational interaction. The galaxy's color profile shows a brighter central area and a slightly bluer outer region, perhaps indicating regions of ongoing star formation. 
