The galaxy presents as a lenticular or possibly a spiral galaxy seen at a relatively high inclination. The galaxy's morphology appears smooth, exhibiting a higher concentration of light toward its center, suggesting a prominent bulge. The color profile indicates a blue hue, particularly noticeable in the disk region, which may imply recent or ongoing star formation activity. The object appears elongated, with a definite major axis significantly longer than its minor axis. Based on the observed morphology, there are no obvious signs of recent major merger events, however, there is some subtle irregularity visible, which could be indicative of minor tidal interactions or internal disturbances. Overall, the structure is well-defined, and the lack of substantial dust lanes supports the assessment of it potentially being an inclined spiral, but this cannot be definitively determined from the data given.
