The galaxy presents as a single, consolidated luminous object with a generally elliptical morphology. Its core region exhibits a bright, concentrated glow, suggesting a high density of stars within. The light gradually fades as it extends outwards from the center, forming a diffuse halo. There is a slight elongation or cigar shape to the galaxy, but it appears mostly rounded. The color profile is primarily yellow, trending toward red, which could indicate an older stellar population or significant dust obscuration. The galaxy lacks any distinct spiral arm structures or prominent star-forming regions visible in this image, instead presenting a smooth and relatively uniform structure. I observe no signs of ongoing major mergers or significant tidal disturbances, although there may be minor irregularities in the outer halo's intensity profile.
