The galaxy presents an elliptical morphology, exhibiting a smooth, featureless appearance. The central region shows a concentrated, bright core, surrounded by a more diffuse halo. The color profile is suggestive of an older stellar population dominating the central bulge, with a yellowish-orange hue. There is some evidence of bluer, possibly younger stellar populations within the disk, but the overall color profile is indicative of a relatively passive galaxy. The galaxy appears undisturbed, with no significant tidal features or signs of recent merger activity visible. The axial ratio indicates a slightly flattened structure.
