The galaxy presents as a slightly elongated, centrally concentrated object. The light distribution appears relatively smooth, with a bright central bulge region that dominates the overall luminosity. The galaxy exhibits a subtle color gradient, transitioning from a bluer hue towards the core to a redder hue in the outer regions. There is little evidence of distinct spiral arms or significant dust lanes, although some faint, irregular features could be present in the outskirts. The overall morphology suggests an elliptical or lenticular galaxy, potentially with ongoing or recent star formation, albeit at a moderate level. There appears to be no major signs of ongoing merger events or significant tidal disturbances.
