The galaxy presents as a relatively smooth, elliptical morphology. The color profile suggests a dominant population of older stars, indicated by the reddish-yellow hue, particularly concentrated towards the galactic center. There's a gradual fading of light intensity from the core outwards, contributing to the smooth appearance. No distinct spiral arm structures or prominent dust lanes are visible within the galaxy's structure. The overall shape approximates a circular form, with a minor degree of ellipticity. There is no evidence of significant tidal disturbances or ongoing major merging events within the immediate vicinity.
