The galaxy presents an elliptical morphology, exhibiting a smooth and concentrated light distribution. It appears elongated, displaying an axis ratio suggestive of an E4 to E5 classification on the Hubble sequence. The central region showcases a bright, prominent core, potentially indicative of an active galactic nucleus or a dense concentration of stars. The galaxy’s color profile exhibits a yellowish-orange hue, implying a stellar population dominated by older, redder stars. There is little evidence of significant dust lanes or spiral arm structure. A slight asymmetry can be observed, possibly related to a minor gravitational disturbance, but there are no clear signs of an ongoing major merger or tidal features.
