The galaxy presents a somewhat elliptical morphology, with a high degree of smoothness. The central bulge appears bright and concentrated, contributing significantly to the galaxy's overall luminosity. A faint disk component is subtly suggested, oriented nearly edge-on. Some subtle irregularities are present within this disk, potentially indicating minor disturbances, such as a tidal interaction. Colors are primarily consistent with a population of older stars, indicated by the redder hue, although there is a hint of bluer light near the disk suggesting a relatively low level of on-going star formation. The estimated size appears relatively compact given its distance.
