The galaxy presents a generally smooth, elliptical morphology. It exhibits a concentrated central bulge that appears quite bright, indicating a high density of stars in the core. The overall color is slightly reddish, suggesting an older stellar population with relatively little ongoing star formation. There is a subtle extension of the galaxy's light in one direction, but this is not well-defined; this could indicate the presence of a faint disk or tidal feature, but the resolution is not sufficient to make a definitive assessment. There is no clear evidence of spiral arms or significant dust lanes. The galaxy appears relatively isolated, with no obvious signs of interaction with other galaxies in its immediate vicinity.
