The galaxy presents as a relatively elongated system, exhibiting a moderately flattened profile. It appears to be an edge-on or nearly edge-on disk galaxy. A prominent central bulge is visible, displaying a concentrated luminosity. The disk component shows a diffuse, extended morphology, fading gradually from the central bulge. There is evidence of internal structure within the disk, but individual features are not clearly resolved. The overall color suggests a mix of stellar populations, with a possibly older, redder population dominating the bulge and a somewhat bluer population present in the disk. There is no apparent indication of a strong interaction or recent merger event, with the galaxy exhibiting a generally undisturbed structure.
