The galaxy presents a primarily smooth morphology, with a slightly elongated, oval shape. Its color profile indicates a population of older stars, with a dominant reddish-orange hue in the central region, suggesting a significant population of evolved stars. The galaxy displays a subtle disk-like component, but no well-defined spiral arms are apparent. There are some indications of minor disturbances in the galaxy's structure, possibly hinting at past interactions or minor mergers. The overall color and smooth texture suggests that star formation is present, though not at an extremely high rate. The galaxy appears moderately massive.
