The galaxy appears as a single, luminous object with a smooth, elliptical morphology. The core exhibits a higher surface brightness, indicated by a concentrated, bright region at the center. The light distribution is generally symmetric, with a gradual decline in luminosity moving outwards from the center. There is a possible secondary concentration of light slightly offset from the main center which could suggest a minor disturbance or ongoing merger. The galaxy presents a yellowish-orange hue, suggesting a population dominated by older stars and a low rate of active star formation. The galaxy’s overall structure appears well-defined despite the potential disturbance, with a generally rounded shape.
