The galaxy presents a smooth, elliptical morphology. It appears to be largely featureless, lacking prominent spiral arms or significant dust lanes. The central bulge is prominent and exhibits a concentrated brightness, suggesting a high stellar density. Moving outward from the core, the luminosity gradually decreases, fading into a diffuse halo. The overall color profile suggests a relatively old stellar population, with a noticeable absence of bright blue star-forming regions. There may be a slight color gradient visible, with the core exhibiting a subtly redder hue compared to the outer regions. The galaxy's elongated shape indicates a moderate degree of ellipticity, appearing cigar-shaped. There's no obvious evidence of ongoing mergers or tidal interactions in the immediate vicinity.
