The galaxy presents an overall elliptical morphology, exhibiting a centrally concentrated luminosity profile. The core is a bright, yellowish-white, suggesting an older stellar population. Fainter, bluish hues appear at the edges of the galaxy, hinting at the presence of younger, hotter stars in the outskirts. The galaxy appears relatively smooth in texture, with no distinct spiral arm structures or prominent dust lanes visible. There is a slight elongation in its shape, trending toward a cigar-like appearance, but mostly appears somewhere in between round and elliptical. No significant tidal features or distortions are observed in the immediate vicinity, suggesting the absence of any major ongoing merger events or significant gravitational interactions.
