The galaxy presents as a moderately luminous object with a somewhat elliptical morphology. It is characterized by a central, bright, diffuse bulge or core region, possibly indicative of an older stellar population. The overall color profile suggests a moderate redshift, with a redder hue apparent in the inner regions potentially due to dust extinction or older stars. A faint, extended disk appears to surround the central bulge, though the structure is not well-defined. The galaxy shows possible evidence of minor disturbances or interactions, perhaps with subtle tidal features or asymmetries in the outer regions, yet the main structure appears relatively undisturbed. No clear spiral arm structures or prominent star-forming regions are visible. The galaxy's relatively smooth appearance indicates that it is likely a transition galaxy between a spiral and elliptical galaxy. The mass and star formation rate show that this galaxy has a high mass but very low star formation. 
