The galaxy presents as a centrally concentrated object, exhibiting a generally smooth morphology. The primary color appears to be a yellow-orange hue, indicative of an older stellar population. There is some evidence of a subtle disk structure, although not sharply defined. A faint greenish tint is noted in regions outside the core, potentially suggesting some ongoing, albeit limited, star formation. No significant tidal features or signs of a major ongoing merger are immediately apparent, although a minor disturbance cannot be entirely ruled out. The galaxy displays a moderately elliptical shape, leaning towards being somewhat rounded.
