The galaxy presents a generally smooth, elliptical morphology. The light distribution appears highly concentrated towards the center, with a gradual decrease in intensity outwards. The galaxy exhibits a yellowish hue, suggesting a population of older stars with lower levels of ongoing star formation. There is no evidence of prominent spiral arms or a well-defined disk structure. The galaxy appears relatively isolated with no obvious signs of tidal disturbances or interactions with neighboring galaxies. The isophotes are largely concentric and round.
