This galaxy exhibits an overall elliptical morphology. The light distribution appears smooth and concentrated towards the center, indicating a significant bulge component. The galaxy appears elongated, with a cigar-like shape. There is no clear evidence of spiral arms or distinct features such as dust lanes. The color profile suggests a population of older stars, evidenced by the reddish-yellow hue, though there is some blue scattered throughout the galaxy which indicates at least some younger stars. There is no apparent evidence of ongoing major merger events. The galaxy displays no signs of active galactic nuclei (AGN) or particularly high star formation.