The galaxy presents as a single, concentrated object with a generally smooth appearance. Its shape is approximately round, with a slight elongation or ellipticity noticable in the overall form. The central region exhibits a brighter, more intense luminosity, suggesting a significant concentration of stars or an active galactic nucleus. Moving outward from the core, the light gradually diminishes, lacking distinct spiral arms or other complex structures. There is a subtle colour gradient observed, shifting from a yellowish-white in the central core to a slightly redder hue in the outer regions. No prominent dust lanes or signs of ongoing major mergers are evident. The galaxy shows no signs of significant disturbances.
