The observed galaxy exhibits a distinct elliptical morphology. Its light distribution presents a smooth, centrally concentrated profile, with luminosity decreasing steadily from a bright, yellowish core. The galaxy's shape is elongated, approximating a cigar shape. There is a slight asymmetry in the outer regions, possibly suggesting a minor gravitational disturbance or interaction. The overall color profile transitions from the yellowish core to redder hues in the outer regions. No prominent spiral arms or distinct features like dust lanes are discernible. The galaxy appears relatively isolated, without any obvious companion galaxies or ongoing major merging events.
