The galaxy presents as a relatively smooth, elliptical object. Its morphology is dominated by a centrally concentrated bulge, exhibiting a bright, yellowish-white glow. The light gradually diffuses outwards from the core, indicating a decreasing stellar density with radial distance. There's a lack of defined spiral arm structures or prominent dust lanes, suggesting a primarily older stellar population. The galaxy appears quite round in shape, with no obvious signs of significant tidal disturbances or ongoing major merging events. Subtle asymmetries are visible, however they don't appear substantial enough to classify as a violent interaction. Overall, the galaxy is an example of an early-type system that shows little recent star formation activity.
