The galaxy presents as a moderately luminous, elongated structure, suggestive of an elliptical morphology, though some disky features cannot be ruled out. The central region displays a higher surface brightness and exhibits a yellowish hue, possibly indicating an older stellar population and diminished star formation activity within the core. Moving outwards, the color transitions to a slightly bluer, less concentrated region, hinting at the presence of younger stars and ongoing star formation in the outer regions, albeit at a lower rate than in typical spiral galaxies. The overall shape is cigar-like, with a lack of distinct spiral arms or other prominent features, indicating that if the galaxy had spiral arms previously, it could have gone through a merger and begun settling into its observed shape. There are no significant signs of tidal disturbances or ongoing interactions with other galaxies.
