The galaxy presents as an elongated, cigar-shaped structure. It exhibits a generally smooth morphology, with no readily apparent spiral arms or distinct features. The light distribution suggests a centrally concentrated luminosity profile, fading gradually towards the outer edges. A slight color gradient is observed, with the central region appearing subtly bluer compared to the outer regions which are redder. This might indicate the presence of younger stellar populations and ongoing star formation in the core, whereas the outer regions might be dominated by older, redder stars. No signs of major disturbances, tidal tails, or merging activity are evident in the image.
