The galaxy presents a predominantly smooth morphology, with a high degree of central concentration as evidenced by the bright, compact core. A faint disk-like structure appears to surround the core, exhibiting a slightly more irregular distribution of light. The overall color is yellowish-white, with a subtle bluer hue detectable in the outer regions of the disk, possibly indicating ongoing star formation. No prominent spiral arms or bar structures are readily apparent. There are no clear signs of major mergers or significant tidal disturbances, although slight asymmetries in the outer disk may suggest minor interactions or past accretion events. The galaxy appears relatively isolated within its immediate environment.
