The galaxy presents as a predominantly smooth, centrally concentrated object. The light profile suggests an elliptical morphology, being largely featureless with no discernible spiral arms or prominent dust lanes. The central region exhibits a brighter, more concentrated luminosity, likely indicating a dense stellar population or a possible active galactic nucleus. The object's shape appears nearly circular, with only a slight deviation towards an elongated form. There is some bluer color towards the periphery of the galaxy, suggesting that there are newer populations of stars in the outer regions. The galaxy does not appear to be undergoing a major merger, although there is evidence of a potential minor disturbance in the galaxy's structure.
