The galaxy presents as a moderately bright, elongated structure with a significantly brighter central bulge. The overall shape is somewhat cigar-shaped, suggesting a possible elliptical morphology, although a highly inclined disk cannot be ruled out. The light distribution appears relatively smooth, lacking distinct spiral arms or prominent features. A faint blueish hue is present on the edges of the galaxy, suggesting that it may have some star formation. There is no apparent interaction with any nearby galaxies and it appears to be undisturbed. The color distribution suggests an older stellar population dominating the central regions, transitioning to younger, bluer stars on the outer edges.
