The galaxy presents as an elliptical morphology, exhibiting a generally smooth texture with a high degree of central concentration. The light distribution is relatively uniform, lacking prominent spiral arm structures or distinct dust lanes. The central region is significantly brighter and appears to be yellowish, suggestive of an older stellar population. The overall shape is somewhat elongated, but not significantly so. There are no obvious signs of ongoing mergers or major tidal disturbances, although there is some minor asymmetric disruption present. Color gradients across the galaxy are relatively subtle, transitioning from a yellow hue in the core to a slightly redder hue in the outer regions. The galaxy's profile appears fairly well-defined, indicating a relatively settled and evolved system.
