The galaxy appears to be an elliptical or lenticular type, exhibiting a smooth, featureless morphology. Its overall shape is largely circular, with no apparent spiral arms or bar structures. The color distribution indicates an older stellar population, with a higher concentration of redder stars, although there appears to be some recent star formation contributing a bluer hue within the central region. There is no evidence of any major disturbances or tidal features suggesting a recent merger event, although some minor irregularities in the outer regions cannot be ruled out. The galaxy appears relatively isolated within its environment, showing no signs of interactions with neighboring galaxies.
