The galaxy presents a generally smooth, elliptical morphology. There is a high degree of central concentration, with light intensity decreasing gradually towards the outer edges. The galaxy appears mostly featureless; no distinct spiral arms, bars, or dust lanes are readily apparent. The color profile suggests an older stellar population, with a yellowish-red hue dominating the galaxy's composition. There is no sign of an active galactic nucleus or significant ongoing star formation activity. The galaxy's shape appears close to round. There is no major or minor disturbances suggesting there has not been any galactic mergers in its recent history. 
