The galaxy presents an overall elliptical morphology, although not perfectly spherical. It appears somewhat flattened, tending towards a more oblate shape. A smooth light distribution characterizes the central region, with a concentrated core. There are hints of some disturbed features, such as subtle asymmetries or irregularities in the outer regions which may indicate some tidal disturbances. There are areas of apparent star formation, possibly from interactions with another galaxy. The light color of the galaxy is dominated by a brighter bluer hue in the center, transitioning to a redder color near the outskirts. This suggests active star formation in the central regions which tapers off near the edge of the galaxy. There is evidence of a significant population of evolved, redder stars in the galaxy's periphery. There appear to be no well defined spiral arms or a prominent disk structure. The galaxy exhibits characteristics consistent with a relatively massive system, as indicated by its overall size and luminosity.
