The galaxy appears to be a relatively smooth, elliptical type. It exhibits a generally cigar-shaped morphology. The light distribution suggests a centrally concentrated bulge with a gradual decrease in luminosity towards the outer regions. There is a hint of a disk-like structure, although it is not a prominent feature. No distinct spiral arms or significant dust lanes are discernible. The color profile indicates a population of older stars, with a relatively redder overall hue. There's no clear evidence of active star formation regions within the visible spectrum, nor do there seem to be ongoing major merger events or tidal disturbances significantly altering its form. The shape of the galaxy is somewhat elongated.