The galaxy appears to be a moderately luminous, elongated system. Its morphology seems primarily smooth and spheroidal, without any obvious spiral arm structure or prominent dust lanes. There is a color gradient within the galaxy, the central region appears more yellow/white, which might suggest an older stellar population, while the outer regions possess slightly bluer hues, that could indicate the presence of younger, hotter stars. The galaxy's elongated shape suggests it is either an elliptical galaxy with some degree of ellipticity or a lenticular galaxy seen nearly edge-on. There is no strong evidence of any major ongoing merger activity or significant tidal disturbances in the image.
