The galaxy presents a largely smooth, elliptical morphology. A concentrated central bulge is evident, transitioning into a more diffuse halo region. The light distribution appears to be relatively uniform, with no prominent spiral arms or significant dust lanes visible. The color profile suggests a population of older stars, exhibiting a redder hue overall, with the center being a bright yellow color. There's little evidence of ongoing star formation within the visible spectrum, as indicated by the lack of blue or ultraviolet emission. There might be a slight warp in the galaxy suggesting a past merger event, but it's mostly smooth.