The galaxy presents a largely elliptical morphology, appearing more elongated than circular. Its central region exhibits a concentrated, bright core with a yellowish-orange hue, suggesting a population of older stars. Moving outward from the core, the color transitions to a slightly bluer tint, hinting at possible, but diminished, star formation activity in the outer regions. The galaxy's overall structure appears relatively smooth, with no obvious signs of major disturbances such as tidal tails or strong asymmetries. Faint, diffuse features, possibly faint spiral arms or dust lanes, are subtle and require closer inspection to confirm. There are some indications of disturbances, however these are minor. The observed morphology is generally consistent with an intermediate disk galaxy.
