The galaxy presents an overall elliptical morphology, elongated in shape, but not exceedingly so. The light is concentrated toward the central region, indicating the presence of a bulge. The galaxy exhibits a smooth appearance, with the majority of its light appearing diffused and not indicative of well-defined spiral arms or intricate dust lanes. There appears to be a minor disturbance in the symmetry of the galaxy, possibly indicating a small interaction or tidal effect, but no major merger is indicated. Color gradients are subtle, shifting toward redder hues in the central bulge region and slightly bluer tones toward the outer regions, suggesting ongoing, but slow, star formation. Based on the color and morphology, this galaxy may be classified as an early-type spiral or an elliptical galaxy with a modest amount of on-going star formation.
