The galaxy presents as a single, relatively smooth object with a concentrated central region. The morphology appears primarily elliptical, exhibiting a largely featureless profile, with a smooth transition from the core to its outer regions. The galaxy displays a slight elongation, deviating somewhat from a perfectly circular form, possibly suggesting it is of type E4 or E5 on the Hubble sequence. The color profile shows a yellowish to reddish hue, indicating an older stellar population with reduced ongoing star formation. The galaxy exhibits no apparent spiral arm structures, dust lanes, or tidal tails, consistent with it being a mature system, where any past mergers have fully integrated. There is no strong evidence of active galactic nucleus activity observable in this image, although this cannot be definitively ruled out. It has a compact but not stellar-like core.
