The galaxy presents as a centrally concentrated system, exhibiting a relatively smooth morphology with a dominant spheroidal component. It appears largely featureless, lacking prominent spiral arms or strong dust lanes. The core region displays a bright, concentrated luminosity, suggesting a high stellar density or the presence of an active galactic nucleus. The radial light profile indicates a gradual decrease in surface brightness away from the center, implying a diffuse halo extending beyond the core. A subtle color gradient is observed, transitioning from a yellowish core to slightly redder outer regions. This could be indicative of older stellar populations dominating the outer parts of the galaxy, while younger, bluer stars are more concentrated in the center, or it could indicate a higher amount of dust in the outer regions of the galaxy. There is little visual evidence of ongoing major merger activity or significant tidal disturbances. Minor asymmetry in the outer halo might suggest a past interaction or accretion event, but further investigation is required.