The galaxy presents as a relatively smooth, elliptical morphology. There appears to be minimal structural disturbance or tidal features indicative of recent major mergers, although there might be very faint signs of a minor interaction. The galaxy exhibits a color gradient, transitioning from a bluer central region to redder hues in the outer regions, indicative of a decreasing presence of younger stars further from the galactic center. The overall shape is moderately elongated, deviating slightly from a perfectly circular profile. The light distribution is concentrated towards the center, suggesting a substantial bulge component. Star formation is occurring within the galaxy, based on the overall bluer hue, but at a comparatively lower rate.
