The galaxy appears as an elliptical or lenticular type, exhibiting a smooth, largely featureless morphology. There is no apparent spiral structure or prominent dust lanes. The light distribution is concentrated towards the center, with a gradual decrease in intensity outwards. The central bulge region is moderately bright and slightly elongated. The galaxy exhibits a yellowish hue, suggestive of an older stellar population with minimal ongoing star formation. There are no signs of tidal disturbances or ongoing mergers with other galaxies.
