The galaxy presents a generally smooth, elongated morphology, suggesting a classification as a possible lenticular or elliptical galaxy. The central region exhibits a yellowish-orange hue, indicative of an older stellar population. The light appears concentrated towards the center and fading out gradually towards the edges. A slight asymmetry, perhaps due to a minor gravitational interaction, is present. The galaxy has a very slight bluer tint around its edge indicating some young star formation. Based on the color and the shape the galaxy appears to be a disk galaxy observed nearly edge-on.
