This galaxy presents as a relatively smooth, centrally concentrated object. The light profile appears mostly uniform, exhibiting a gentle falloff in intensity from the core outwards. The core appears to have a yellowish/whitish hue, potentially indicating an older stellar population or a lack of significant dust obscuration in the nuclear region. No distinct spiral arms or prominent features are discernible. There may be subtle asymmetry, but the overall structure suggests a system nearing spheroidal morphology. No obvious signs of recent or ongoing major merger events are apparent, though minor tidal disturbances cannot be entirely ruled out based on this single image. The galaxy displays colors consistent with star formation, with the presence of some intermediate to young stars. The estimated luminosity suggests it is a moderately luminous galaxy.
