The galaxy presents as a slightly elongated elliptical form. Its color profile appears relatively uniform with a bright central concentration, suggesting an older stellar population dominating the galaxy's overall light emission. There appears to be little evidence of spiral arms or significant dust lanes within the observed spectral range. The galaxy's smooth morphology indicates a system where star formation may be less active overall or has ceased entirely. Its cigar-shaped morphology reveals the galaxy is likely viewed at an oblique angle, but it is not at an extreme angle.
