The galaxy presents as a single, luminous spheroid with a concentrated, bright central region indicative of a substantial galactic nucleus. The color profile exhibits a shift towards the redder end of the spectrum, suggesting a population of older stars dominating its stellar content. The overall morphology appears smooth with no discernible spiral arms or significant dust lanes. It exhibits a generally elliptical shape, appearing mostly round with some indication of elongation along one axis. There are no obvious signs of interaction with other galaxies, such as tidal tails or distortions, pointing to a relatively isolated system that is not currently undergoing a major merger event.
