The galaxy presents as a lenticular, or possibly an elliptical galaxy, exhibiting a generally smooth morphology. Its overall shape is elongated, with a cigar-like appearance. The central region displays a higher concentration of light, gradually fading towards the outer edges of the galaxy. The color gradient suggests the core might contain older stellar populations, while the disk shows signs of more recent star formation. No distinct spiral arms or significant dust lanes are apparent in the image. There is no clear evidence of major tidal disturbances or ongoing mergers. The galaxy appears relatively isolated, without any immediate neighboring galaxies visibly interacting with it.
