The galaxy presents a generally smooth morphology with a slight elongation, appearing more lenticular than spiral or elliptical. Its color profile reveals a concentration of yellow-white light in the central region, suggesting an older stellar population. A gradual decrease in light intensity is observed moving outwards from the core, fading into a faint blue halo. No distinct spiral arms or dust lanes are visible, indicating a lack of significant ongoing star formation. The overall structure shows no major disturbances or signs of recent mergers, with only subtle asymmetries potentially hinting at minor gravitational interactions.
