The galaxy presents a generally smooth morphology, lacking defined spiral arms or a prominent disk structure. It exhibits a cigar-like shape, with an elongated, ellipsoidal form. A bright central bulge region is apparent, gradually fading into the outer regions. The color profile suggests a concentration of older stellar populations in the core, with a shift towards slightly bluer hues in the outskirts. This color gradient could indicate ongoing, albeit subdued, star formation activity in the outer regions compared to the core. There are no obvious signs of major mergers or significant tidal disturbances in this image. Minor disturbances in the outer halo cannot be excluded.
