The galaxy presents a generally smooth, elliptical morphology. The light distribution appears centrally concentrated, with a gradual decline in intensity towards the outer regions, characteristic of an early-type galaxy. No distinct spiral arms or bar structures are apparent. The galaxy exhibits a relatively round shape. There is no evidence of a significant ongoing merger or major tidal disturbance. However, there appears to be a slight irregularity in its otherwise smooth structure, which may be indicative of a minor disturbance or recent interaction. The color is yellowish and has a hint of redness, indicative of an older stellar population. I estimate the diameter to be approximately 6 kpc, and the mass to be high, with moderate to low star formation.
