The galaxy appears to be a relatively luminous system, exhibiting a slightly elliptical morphology. The light distribution is dominated by a smooth, centrally concentrated component, suggesting a significant bulge. There is a faint hint of a surrounding disk, but distinct spiral arms are not readily apparent. The color of the galaxy appears to be trending towards the redder end, indicating a higher proportion of older stellar populations, with perhaps low on-going star formation. Based on the lack of strong morphological disturbances, the system appears relatively undisturbed. There appears to be no distinct features, like bars or rings, in the galaxy. No sign of an active galactic nucleus is present either.
