This galaxy appears to be a relatively smooth, elliptical galaxy with a concentrated central bulge. It exhibits an overall yellowish hue, suggesting an older stellar population with fewer young, massive stars. There is a suggestion of a faint tidal stream or extended structure extending from the galaxy, potentially indicating a past minor merger event or tidal interaction. The main body is somewhat round with only a slight deviation from a purely circular shape. There is a central concentration of light, likely due to a dense nuclear region or a supermassive black hole. The galaxy does not appear to show any significant signs of ongoing star formation or prominent spiral arms. Overall, the object likely has a high mass and a relatively low star formation rate.
