The galaxy presents a mixed morphological classification, appearing largely smooth but with some discernible features. It has a mostly elliptical shape with a bright, concentrated central region, suggesting an older stellar population. The galaxy exhibits a yellow-orange hue, indicating a lower rate of ongoing star formation. Some bluer regions are present, indicating some more recent star formation occurring outside of the central region. There are also minor disturbances visible in the galaxy's structure, suggesting a possible minor interaction or tidal disruption. The overall impression is of a galaxy undergoing a transition from a disk-dominated system to a more spheroidal form, with traces of past merger events still visible.
