The galaxy presents as an elongated, elliptical shape, appearing cigar-shaped. The light distribution is generally smooth, showing a central bulge that fades into a diffuse disk. There is an apparent lack of strong spiral arm structure, though some faint color variations suggest underlying features within the disk. Color gradients suggest older stellar populations are located in the central regions, while the outer edges of the galaxy appear to show bluer hues, potentially indicating a degree of ongoing star formation. The disk exhibits a noticeable tilt relative to our line of sight. The galaxy does not appear to be undergoing any major merging events or strong tidal disturbances.
