The galaxy presents as a primarily smooth, elliptical-like structure. Its overall shape is elongated, with a cigar-like appearance rather than a perfectly circular form. The central region exhibits a brighter, concentrated luminosity, indicating a possible core or bulge. The light distribution appears relatively even and diffuse, with no obvious spiral arms or distinct features. Color gradients suggest a redder central region possibly indicating an older stellar population. The edges of the galaxy fade smoothly into the background, without sharp boundaries or tidal tails. There is a hint of blueish coloration at the edges. There's no apparent indication of recent major merger activity or significant disturbance.
