The galaxy presents a morphology suggesting an elliptical or lenticular classification, with a notable absence of well-defined spiral arms. Its central bulge is prominent and appears relatively smooth, exhibiting a concentrated luminosity profile. Faint extensions or tidal features are visible, potentially indicating past or ongoing interactions with other galaxies. The galaxy's overall color is indicative of an older stellar population with a low star formation rate. The image does not reveal substantial dust lanes or active star-forming regions, which further supports the conclusion that star formation activity is minimal. There may be a minor merger happening with a smaller satellite galaxy on the left side of the galaxy.
