The galaxy presents as an edge-on disk galaxy with a distinct central bulge. The bulge appears yellowish-white in color, indicative of an older stellar population. The disk component is visible as a faint, elongated structure extending outward from the bulge on either side. There is a suggestion of a dust lane bisecting the disk, although the resolution is not high enough to definitively confirm this. The galaxy exhibits a relatively smooth morphology, with little evidence of strong spiral arm structure or significant tidal disturbances. Overall, the galaxy appears to be a relatively quiescent system, consistent with a later Hubble type. The disk component shows a bluer hue than the central bulge, potentially indicating ongoing star formation.
