The galaxy appears as a single, relatively smooth object, exhibiting a concentrated central bulge and a diffuse, indistinct disk. The color profile suggests a population of older stars, with a redder hue overall, indicating less ongoing star formation. There is a slight elongation in its shape but lacks any prominent spiral arms or bar structures. There is no visible evidence of recent or ongoing mergers, tidal tails, or any major disturbances in the surrounding area. The object seems relatively undisturbed and evolved.
