The galaxy presents with a notable central bulge, exhibiting a concentrated, yellowish hue that suggests an older stellar population. Surrounding the bulge, a fainter, bluish disk is observed. The disk appears somewhat disturbed or irregular, lacking a clearly defined spiral structure. The morphology suggests a galaxy undergoing, or recently having undergone, some form of interaction or internal process that has disrupted the overall structure. The galaxy has a estimated size of 8.2 Kpc. There are hints of faint, diffuse extensions that may indicate tidal features, although more data would be needed to confirm this hypothesis. Overall, the galaxy appears to be in a transitional stage of evolution.
