The galaxy presents an elliptical morphology, though it is not perfectly smooth. Some subtle features suggest a disk-like component oriented at an angle relative to our line of sight. The central bulge appears bright and concentrated, exhibiting a yellowish-white color, likely indicative of an older stellar population. Fainter, bluer hues are visible within the surrounding disk, perhaps hinting at regions of more recent star formation. There is a slight irregularity to the overall shape, possibly due to a minor gravitational interaction or a past merger event. No strong evidence of spiral arms is apparent.
