The object presents as a galaxy at a redshift of approximately 0.315. Morphologically, the galaxy appears elongated, cigar-shaped and inclined with respect to our line of sight, indicating it is likely a disk galaxy viewed edge-on. It exhibits a notable central bulge that is concentrated and bright, with a yellowish-orange hue suggesting an older stellar population. Moving outwards from the bulge, a fainter, bluer disk is suggested, although this feature is poorly resolved in the image. There is little evidence of spiral arm structure, indicating it is a late-type disk galaxy, perhaps a lenticular galaxy or an early spiral with poorly defined arms. There are no obvious signs of major merger activity or strong tidal disturbances. The overall light distribution suggests a relatively smooth morphology, with no prominent star-forming regions or knots visible. Based on color, the galaxy seems dominated by an older stellar population, consistent with a relatively low star formation rate.
