The galaxy presents a largely smooth, elliptical morphology. There is a concentration of light towards the center, suggesting a dense galactic nucleus. The galaxy exhibits a yellowish hue, possibly indicative of an older stellar population with reduced ongoing star formation. Its relatively uniform appearance across the surface does not reveal any prominent spiral arms or significant dust lanes. The overall shape appears somewhat rounded, lacking the elongated, cigar-like appearance sometimes associated with elliptical galaxies undergoing tidal interactions. There's no obvious sign of major mergers or significant disturbances in the overall structure of the galaxy.
