The galaxy presents as a largely homogenous structure with a smooth appearance, indicating a lack of prominent spiral arms or other distinct morphological features. The light distribution is centrally concentrated, with a relatively diffuse and extended halo. Color gradients appear subtle, shifting from warmer hues towards the center to cooler tones in the outskirts, potentially indicative of varying stellar populations or dust content across the galaxy. The overall shape is generally rounded, showing minimal deviation from a circular profile, with no apparent signs of ongoing major mergers or significant tidal disturbances, though minor disturbances cannot be ruled out based on the present image. The galaxy appears relatively isolated, without any clear signs of strong interactions with nearby galaxies.
