The galaxy presents as a spindle-shaped structure with a smooth, diffuse light distribution. The primary axis of the galaxy appears significantly longer than its minor axis, indicating a highly elongated morphology. There is a subtle color gradient visible, with the central region appearing slightly bluer and the outer regions trending towards redder hues. The lack of distinct spiral arms or well-defined dust lanes suggests that this galaxy is likely an elliptical or lenticular type. There is no obvious nuclear bulge, and no significant star formation is apparent upon visual inspection. Based on the overall smooth appearance, this galaxy may be a relatively evolved system with a moderate stellar mass and low star formation rate. The absence of strong tidal features suggests it is not currently undergoing a major interaction. 
