The galaxy presents as a somewhat elongated, lenticular structure. It displays a smooth, centralized bulge that transitions into a more diffuse outer disk. The bulge appears to be composed of older stellar populations, indicated by its yellowish-orange hue. The disk exhibits a bluer color profile, suggesting the presence of younger, hotter stars and ongoing star formation, albeit at a moderate rate. There is little evidence of well-defined spiral arms or significant dust lanes, but there are subtle irregularities in the disk's overall structure. The axial ratio suggests a moderate inclination relative to our line of sight. The lack of any obvious tidal features or close companion galaxies in the immediate vicinity indicates it is likely an isolated system, not undergoing any major mergers or interactions. The overall morphology indicates it is a relatively massive galaxy, likely on the red sequence, with a slowly declining star formation rate.
