The galaxy presents as an elongated, disk-like structure, likely viewed at an oblique angle, but not precisely edge-on. There is a central bulge that appears bright and somewhat smooth, possibly indicative of an older stellar population. The disk component shows some evidence of structure, though not highly resolved. There appears to be a slight asymmetry in the disk with some patchy regions of star formation visible. There may be some minor tidal disturbances or interactions. Overall, this is probably a spiral galaxy with relatively low star formation. The smooth central concentration suggests a mass and specific star formation rate that is consistent with a relatively passive or transitioning galaxy.
