The galaxy presents an overall elliptical morphology, though with some evident disturbances in its structure. The light distribution appears relatively smooth, with a noticeable central concentration of luminosity. Some indications of disruption are present, possibly due to a minor interaction or merger event. There is a significant blue color present within the galaxy, likely indicating the presence of younger stellar populations and ongoing star formation. The galaxy displays a slight elongation and deviation from a perfect circular shape, possibly indicating a transitional state. A small amount of asymmetry is evident, with a slight but noticeable disturbance of the light distribution in one region, suggesting a possible interaction or recent accretion event. The galaxy lacks well-defined spiral arms or a prominent disk, consistent with its smooth light profile and a more spheroidal morphology.
