The galaxy appears to be a relatively small, faint, and elongated object. It presents a subtle bluish tint, with a slight redder component along the central axis. The overall structure hints at a possible edge-on spiral or a lenticular galaxy, though the image resolution limits definitive morphological classification. There is a suggestion of a faint, diffuse disk or tidal feature extending from one side of the galaxy, indicating a potential interaction or disturbance. The central region is not sharply defined. Based on the light profile, it likely has a Petrosian half-light radius of around 10 arcseconds. The color indices suggest that it is a galaxy at moderate redshift. The light distribution does not show a prominent bulge component. There may be an indication of low-level disturbances visible, but the lack of high resolution and low signal-to-noise ratio limit more detailed analysis of such features.
