The galaxy presents an elongated, cigar-shaped morphology, indicative of an elliptical galaxy viewed at an oblique angle or possibly a highly inclined spiral. The central region exhibits a concentrated luminosity, suggesting a prominent galactic bulge. The color profile is generally smooth, with a yellowish-white hue dominating the core, transitioning to a slightly bluer tint towards the outer regions. This color gradient implies older stellar populations concentrated in the center with younger stars towards the outside, as well as ongoing star formation. There is no significant evidence of spiral arms or a distinct disk structure. Minimal distortion suggests no major ongoing merger events or tidal interactions. The galaxy appears to be a relatively isolated system.
