The galaxy presents a generally smooth and concentrated morphology. Its overall shape appears elliptical or lenticular, with no distinct spiral arms or bar structure visible. The light distribution is relatively uniform, although there appears to be a slightly brighter central region, suggesting the presence of a bulge or a more concentrated stellar population at its core. The galaxy exhibits a moderate degree of roundness, neither perfectly spherical nor highly elongated. There is no clear evidence of recent or ongoing major merger activity or significant tidal disturbances in the immediate vicinity, however, there seems to be a slight warp at one end of the galaxy. Overall, the galaxy appears to be a relatively evolved system, potentially undergoing a period of relatively quiescent star formation. The galaxy is moderately luminous.
