The galaxy presents as an elliptical or lenticular type, exhibiting a generally smooth morphology with minimal discernible features. Its overall shape appears oblate, trending towards a more rounded profile than a highly elongated one. The central region displays a high surface brightness, indicating a dense concentration of stars. There's a slight color gradient visible, transitioning from a yellowish-white core to a slightly redder halo. The lack of distinct spiral arms, dust lanes, or prominent star-forming regions suggest a relatively passive galaxy with a low ongoing star formation rate. There is no clear evidence of any major interaction or merging events affecting the galaxy’s structure.
