The galaxy presents a largely smooth, elliptical morphology. Its core is highly luminous, exhibiting a concentrated bright region. Radially outward, the luminosity gradually decreases, with a lack of distinct spiral arm structures or prominent dust lanes. The galaxy appears generally round, with no significant elongation or tidal features suggestive of ongoing major merger activity. There is some evidence of minor irregularities in the outer halo, indicating possible past interactions or internal disturbances, but the overall structure is dominated by its smooth, spheroidal nature. The color gradient suggests a concentration of older stellar populations towards the center, with a bluer, possibly younger population distributed in the outer regions, although this distinction is subtle. The galaxy exhibits a moderate redshift, implying that it is at a substantial distance from our own. The light emitted from the galaxy indicates it is a very massive system with suppressed star formation activity.