The galaxy appears as a moderately luminous, elongated object. It exhibits a relatively smooth morphology, suggesting a lack of prominent spiral arms or irregular features. The light distribution is concentrated towards the center, with a gradual decrease in intensity towards the edges. The central region displays a yellowish hue, potentially indicating an older stellar population. The outer regions appear bluer, possibly indicative of more recent star formation activity. The galaxy appears to be a prolate spheroid, with no signs of significant tidal disturbances or ongoing merger activity apparent in this image.
