The galaxy exhibits an overall smooth morphology with a slightly elongated shape. The central region displays a concentrated, bright core that gradually diffuses outwards. The color profile suggests a transition from a yellowish-white core to a bluer, less intense outer halo. There is a hint of disk structure, although it appears quite disturbed. Based on the observed characteristics, this galaxy appears to be a relatively massive system undergoing relatively low star formation, with some evidence of past or ongoing mergers or tidal interactions.