The galaxy presents as a relatively smooth, elliptical-like object. The central region appears bright and concentrated, exhibiting a yellowish-orange hue, suggestive of an older stellar population. Moving outwards from the core, the light gradually diffuses into a fainter halo. This outer region displays a slightly bluer tint, perhaps indicating pockets of younger stars, though star formation activity appears to be subdued overall. There is a subtle elongation visible along one axis, stopping it from being a perfectly round galaxy. No obvious signs of strong tidal disturbances or ongoing major mergers are apparent. The structure suggests a galaxy evolving in relative isolation with few internal structures.
