The galaxy presents an elliptical morphology, exhibiting a smooth light distribution that suggests an evolved stellar population. A noticeable elongation is present, transitioning from a cigar-shaped to a more rounded form from its core outwards. The galaxy's core region presents a concentrated bright glow, likely comprised of densely packed stars. A minor color variation is visible as a faint and small orange-tinted lobe on one side of the galaxy, which could suggest a small area of recent star formation or potentially a tidal interaction. Overall, the galaxy appears largely undisturbed, showing no significant signs of ongoing major merger activity or violent disturbances.
