The galaxy presents as a centrally concentrated object, exhibiting a roughly elliptical morphology. A smooth light distribution is observed, lacking prominent spiral arm structures or distinct features. The galaxy's core region appears brighter and more compact, potentially indicating a higher density of stars or the presence of an active galactic nucleus. There is a faint, diffuse halo extending outwards from the central region, with a slight blueish color. The blue color is likely indicative of regions of relatively recent star formation within the galaxy. Evidence suggests the galaxy is relatively isolated, with no visually apparent major mergers or tidal disturbances currently affecting its overall structure.
