The galaxy presents an overall smooth morphology. It appears elliptical in shape, with the longest axis oriented approximately horizontally in the image. The core region exhibits a brighter intensity, which gradually diminishes towards the outer edges. The color profile indicates a relatively blue hue, suggesting a presence of younger stellar populations or active star formation within the galaxy. There is faint evidence of minor disturbances or possible tidal features extending from the main galactic body, however these are not significant. No pronounced spiral arm structures or prominent dust lanes are discernible.
