This galaxy presents as a somewhat elongated, cigar-shaped object. The central region exhibits a bright, concentrated luminosity, suggesting a significant stellar density and possibly an active galactic nucleus. The overall color appears to be on the redder side, with a slightly yellowish hue dominating, implying an older stellar population and diminished ongoing star formation within the bulk of the galaxy. Faint, bluer regions can be detected in some areas, which might indicate some limited, more recent star formation. While primarily smooth in appearance, there are hints of a possible disc structure, although this is not very clear. It does not appear to be undergoing a major merger, but there are some subtle signs of minor disturbances in the distribution of the galaxy's light.
