The galaxy presents an elliptical morphology, appearing largely smooth and featureless. The central region exhibits a concentrated, reddish hue, possibly indicative of an older stellar population. Extending outward, there is a more diffuse, greenish halo. This coloration might suggest some ongoing, albeit low, level of star formation within the galaxy. The galaxy appears relatively undisturbed, with no obvious signs of a recent major merger or tidal interactions. Its overall shape is close to round, showing a slight deviation toward a cigar-like form. Any minor distortions can be assumed to be faint and located within the galaxy's boundaries.