The galaxy appears to be a relatively smooth, elongated, disk-like system, potentially a lenticular or edge-on spiral. The central bulge exhibits a concentrated luminosity profile with a yellowish hue, suggesting an older stellar population. Fainter, bluer light extends outwards from the bulge, indicative of more recent star formation within a disk component. There is a slight asymmetry to the outer regions, which could indicate minor tidal interactions, but overall the system does not appear to be significantly disturbed. The lack of distinct spiral arms could suggest a well-mixed disk or the presence of a bar structure oriented along our line of sight.
