The galaxy appears as a centrally concentrated object. It exhibits a predominantly smooth morphology, with a subtle transition in luminosity from the core to the outer regions. The central region is the brightest, gradually fading outwards. The overall shape is moderately elliptical, approaching a circular form, with a slight elongation. There are no readily apparent signs of spiral arms or a pronounced disk structure. There appears to be little to no major merging activity visible. The color profile suggests the presence of an older stellar population; this is indicated by the yellowish hue. Subtle color gradients could imply differences in stellar populations or dust distribution within the galaxy.
