The galaxy presents an overall elliptical morphology, exhibiting a centrally concentrated light distribution that gradually decreases in intensity towards the outer regions. A prominent, bright central bulge is observed, with a yellowish-orange hue, suggesting a population of older stars. The outer disk appears fainter, with a bluer color profile, indicative of younger, hotter stellar populations and ongoing star formation activity. There appears to be only slight indication of spiral arm structure or prominent dust lanes; the structure observed here is indicative of the galaxy being somewhere on the smooth or featured end of the spectrum. It is also exhibiting some indications of minor disturbances. The object displays a moderate redshift, indicating a significant distance.
