The galaxy presents as a centrally concentrated, elliptical-like structure. It exhibits a smooth, relatively featureless morphology, with no apparent spiral arms or distinct dust lanes visible in this imaging. There is a slight elongation observed in the galactic shape, though it is not significantly cigar-shaped. The central region appears to be dominated by older stars, indicated by the presence of yellow to reddish hues, suggesting little to no active star formation. There appears to be a faint blueish glow, primarily around the edges of the central orange light, suggesting more recent star formation, which is a contrast to the bulk of the observed image. Overall, the galaxy has a high degree of symmetry and no obvious signs of major mergers or significant tidal disturbances, indicating its evolution has likely been a primarily internally driven process.
