The galaxy appears as a single, relatively smooth object with a discernible central bulge. The morphology suggests a classification leaning towards elliptical, although some disk-like qualities are present. The concentration of light is highest in the central region, gradually decreasing towards the outer edges. The color profile shows a yellow to orange hue in the core, possibly indicating an older stellar population, while the outer regions exhibit a bluer tint, suggesting the presence of some younger stars. No significant spiral arm structures or dust lanes are immediately apparent in the image. The overall structure is largely undisturbed, showing no clear signs of major mergers or tidal disruptions. Faint hints of a very subtle and diffuse extended halo may be present around the galaxy, but resolution limitations prevent a definitive confirmation. The galaxy presents as moderately luminous.
