The galaxy presents an elliptical morphology, appearing largely smooth and well-rounded. A concentrated central bulge is observed, exhibiting a yellowish hue, likely indicative of an older stellar population. Surrounding the bulge is a fainter, somewhat diffuse halo with hints of bluish tones, suggesting the presence of younger, hotter stars and regions of ongoing star formation, though at a moderate rate. There are no clear signs of spiral arm structures or significant dust lanes. The galaxy appears relatively isolated with no prominent tidal features, suggesting it has not undergone a recent major merger event, though minor disturbances cannot be ruled out. Overall, the galaxy appears to be an elliptical galaxy with a non-negligible amount of recent star formation.
