The galaxy appears to be an elliptical or lenticular type galaxy, exhibiting a smooth, diffuse structure. It displays a slightly elongated, cigar-like shape. The color profile indicates a higher concentration of older stars, with a yellowish-orange hue dominating the light emitted. There is no discernible spiral arm structure or significant dust lane obscuration visible. No tidal features or signs of a recent major merger event are apparent. The galaxy's apparent size suggests a moderately large physical extent, implying a substantial mass. Its overall morphology suggests a relatively evolved system with a low ongoing star formation rate. Minor disturbances cannot be ruled out. 
