The galaxy appears to be a relatively compact system, showing a generally smooth morphology. The light distribution is centrally concentrated, diminishing gradually towards the outer regions, with no obvious spiral arm structure or significant dust lanes visible. The ellipticity is moderate, suggesting a shape that is somewhat flattened but not highly elongated. There is a slight color gradient noticeable, trending from bluer in the central regions to redder in the outer halo, hinting at a declining star formation rate as we move away from the galactic center. There are no signs of major ongoing mergers or strong tidal disturbances, though a slight asymmetry in the outer regions suggests a possible past minor interaction or accretion event. The galaxy appears fairly isolated, with no other nearby galaxies disrupting its form.
