The galaxy exhibits an overall elliptical morphology, with a relatively smooth light distribution. The central region presents a bright, concentrated core that appears yellowish in color, possibly indicating an older stellar population. Extending outward from the core, a faint, flattened disk-like structure is observed, though without distinct spiral arm features. The disk component shows a subtle blueish tint, hinting at the presence of some younger stars and ongoing, but limited, star formation. The galaxy's elongated shape suggests that it is viewed at an inclined angle. There are no obvious signs of recent major mergers or significant tidal disturbances. The overall appearance is consistent with a lenticular or early-type spiral galaxy undergoing relatively low levels of star formation.
