The galaxy appears as a diffuse, elliptical-shaped structure with a relatively smooth texture. The light distribution suggests a centrally concentrated luminosity profile, gradually decreasing towards the outer edges. The color index indicates a bluer hue in the central region, transitioning to slightly redder tones in the outer regions. There is no distinct spiral arm structure or obvious dust lane visible. The overall morphology suggests an older stellar population, but with some ongoing star formation. The galaxy's axial ratio suggests a moderate degree of flattening.
