The galaxy appears as a single, luminous object with a centrally concentrated light profile. The morphology is generally smooth, showing no distinct spiral arms, bar structure, or other complex features typically associated with disk galaxies. It appears nearly circular, suggesting a small degree of visible inclination relative to our line of sight. The colour profile presents a slight gradient; light from the centre of the galaxy is somewhat more red or yellow than the outer regions, which are bluer in colour. This suggests a stellar population gradient, where older, redder stars are more centrally concentrated and younger, bluer stars are located further out. There are no obvious signs of recent or ongoing major mergers or tidal disturbances.
