The galaxy presents a predominantly smooth morphology, exhibiting a somewhat elongated, cigar-shaped structure. A slight blue tint is visible, concentrated towards the central region of the galaxy, suggesting the potential presence of younger stellar populations or ongoing star formation, albeit at a low rate. Faint reddish hues are observed towards the peripheral regions. No prominent spiral arms or distinct disk features are immediately apparent. Overall, the galaxy appears to be relatively undisturbed, with no obvious signs of major mergers or tidal interactions.