The galaxy presents a mostly smooth morphology, with a concentrated central bulge region. This core exhibits a yellowish-orange hue, suggesting an older stellar population. Fainter blueish halos extend outwards from the central region, indicating possible star formation. There are no clear spiral arms, distinct bar structures, or signs of recent major merger events. Slight asymmetry or tidal disturbance might be present on a minor scale. The overall impression is that of a fairly evolved galaxy, with ongoing but modest star formation at the outer parts.
