The galaxy presents as a relatively smooth, centrally concentrated object. Its morphology is generally elliptical, exhibiting a high degree of central bulge dominance with light gradually decreasing radially. The galaxy possesses a yellowish hue in its core, suggesting an older stellar population in the central regions. Fainter blueish light surrounding this core may indicate the presence of younger stars or some degree of ongoing star formation. No distinct spiral arms or prominent dust lanes are visible; its structure lacks any significant features or irregularities. The lack of strong blue light may suggest that star formation is largely suppressed within this galaxy. There's no indication of a merger or tidal disruption, which aligns with the undisturbed morphology of the galaxy.
