The galaxy appears as a relatively smooth, centrally concentrated object. There is little evidence of distinct spiral arms or a prominent disk structure. The overall shape seems to be somewhere between round and slightly elongated. The color distribution suggests a relatively homogeneous stellar population, with a possible slight concentration of bluer stars towards the central region. There is little visual evidence of ongoing major mergers or significant tidal disturbances, though the possibility of minor interactions cannot be ruled out. The galaxy displays a fairly compact morphology. Overall, the galaxy presents characteristics consistent with an elliptical or lenticular galaxy, exhibiting relatively low levels of star formation.
