The galaxy presents as an elliptical morphology, exhibiting a smooth, relatively featureless light distribution. It possesses a concentrated central bulge, characterized by a yellowish-orange hue, suggesting an older stellar population. The galaxy lacks prominent spiral arms or distinct dust lanes. There is a faint, diffuse halo surrounding the central region. The overall shape appears somewhat elongated but is still relatively round. There are no signs of a recent or ongoing major merger event. The galaxy exhibits a minimal amount of recent star formation activity.
