The galaxy appears to be an elliptical type, exhibiting a smooth, relatively featureless morphology. The light distribution shows a centrally concentrated bulge, with a gradual decrease in surface brightness moving outwards. The galaxy exhibits a moderate degree of roundness, neither perfectly spherical nor highly elongated. The color profile is generally consistent, with a hint of redder hues in the central region suggesting an older stellar population. There is no apparent evidence of spiral arms, dust lanes, or ongoing major merger activity. Subtle disturbances or minor asymmetries are not apparent, though the image resolution limits the detection of fine-scale features.