The galaxy appears to be a relatively smooth, centrally concentrated object, potentially elliptical or lenticular in nature. There is no obvious spiral structure or significant dust lane obscuration visible. The color profile exhibits a centrally concentrated yellowish-red hue, indicating an older stellar population dominating the core region. There is a slight bluer tint in the outer regions of the disk, indicating younger stars. The axial ratio suggests a mildly elongated or disk-like morphology, rather than perfectly spherical. Subtle distortions or faint tidal features may be present, suggesting possible past or ongoing interactions with another galaxy. Overall, this galaxy appears to be a rather massive galaxy with moderate star formation.
