The galaxy presents as a centrally concentrated system with a generally elliptical morphology. The central region exhibits a bright, yellowish-white core indicative of an older stellar population, with a slight reddish tinge. Surrounding the core, the galaxy displays a more diffuse, bluish halo. This suggests ongoing, or recent, star formation in the outer regions. While mostly smooth, the galaxy shows a subtle, elongated shape, trending toward a cigar-like morphology. No strong signs of major disturbances are present, suggesting a relatively isolated evolutionary path. There is a slight asymmetry with the distribution of light, hinting at possible minor gravitational interaction, or internal dynamic processes at work.
