The galaxy presents as a lenticular or possibly an edge-on spiral galaxy, observed at a redshift of approximately 0.15. It exhibits a somewhat elongated morphology. There is a noticeable color gradient, with a bluer, brighter region at one end and a shift towards redder hues towards the central region and the opposite end.

The brighter end might indicate a region of more active star formation, while the redder regions are likely indicative of an older stellar population. The overall structure appears relatively smooth, though higher resolution imaging would be needed to discern any finer details such as spiral arms or dust lanes. There is no clear evidence of a prominent bulge. The galaxy does not appear to be undergoing a major merger. The overall impression is that of a relatively evolved galaxy.
