The galaxy presents as a relatively smooth, elliptical-like structure. The central region exhibits a high concentration of light, suggesting a prominent galactic nucleus. The overall color profile is dominated by yellow-red hues, indicative of an older stellar population with relatively little ongoing star formation. The galaxy appears somewhat rounded in shape, with no obvious signs of spiral arm structures or significant disturbances from mergers. There is a single nearby object exhibiting a red hue that is likely either a foreground star, a background galaxy, or another feature, but is not a part of the galaxy being analyzed.
