The galaxy presents as a relatively compact and unresolved object. Its overall morphology appears smooth, lacking any distinct spiral arm features or prominent dust lanes. The color gradient suggests a concentrated, yellowish core that diffuses outward to a less intensely colored halo or outer region exhibiting a slightly bluer hue. The light distribution implies a higher concentration of older stellar populations within the core, with some evidence of ongoing, albeit subdued, star formation in the outer regions. There is no obvious visual evidence of a major merger event or significant tidal disturbances, although minor disturbances cannot be ruled out based on this image alone. The galaxy appears to be neither perfectly spherical nor highly elongated, possessing an intermediate ellipticity. Overall, it is most likely an elliptical or lenticular galaxy at an approximate redshift of 0.09.
