The galaxy appears to be an elliptical or lenticular galaxy, exhibiting a flattened, disk-like structure with a relatively smooth, featureless morphology. The light distribution is centrally concentrated, with a gradual decrease in intensity towards the outer regions.

There is a noticeable color gradient, with the central region appearing more red, potentially indicating an older stellar population, while the outer regions are more blue, indicative of younger stars and regions of active star formation.

There is no visible spiral structure or bar feature, consistent with an early-type galaxy classification. The disk is moderately inclined with a major to minor axis ratio of approximately 2:1. There is no clear evidence of tidal features or interactions with other galaxies, suggesting it is a relatively isolated system.
