This galaxy presents a predominantly smooth morphology, with a high degree of central concentration. The overall shape appears nearly round. There's little evidence of spiral arm structure or significant dust lanes. The central bulge exhibits a yellowish hue, suggesting an older stellar population. The surrounding halo fades gradually, displaying a slightly bluer color, possibly indicating the presence of younger stars, even if star formation is happening at a very low rate. The galaxy does not appear to be undergoing any major merging activity. Close inspection does not reveal any tidal tails or other significant distortions.
