The galaxy presents a morphology that is neither purely smooth nor distinctly featured. Its appearance suggests a significant degree of central concentration with a brighter, somewhat diffuse core. The overall color profile indicates a relatively evolved stellar population, exhibiting a yellowish-orange hue. There is a slight asymmetry evident in the galaxy's structure, possibly indicative of a past or ongoing minor interaction. The isophotes appear somewhat irregular, suggesting the presence of tidal disturbances or recent accretion events. While the primary body of the galaxy is discernible, there are no clear spiral arm structures or prominent star-forming regions visible in this imagery. The galaxy's halo appears faint and indistinct, blending gradually into the background sky.
