The galaxy exhibits a morphology that is neither purely smooth nor clearly exhibiting spiral arms. It presents an overall elliptical shape but with some visible substructure suggesting a disk component. The central bulge appears luminous with a yellowish-white hue, indicative of an older stellar population. Surrounding the bulge, the galaxy exhibits a bluer color distribution, possibly indicating regions of more recent star formation. The outer regions appear somewhat irregular and show signs of minor disturbances, with a slightly clumpy texture suggesting potential past interactions. This suggests a possible recent minor merger or tidal interaction with a nearby galaxy. The galaxy has a moderate redshift and is considered a fairly massive galaxy with relatively low star formation activity.
