The galaxy presents as an elongated, cigar-shaped structure. A prominent central bulge is observed, exhibiting a smooth, concentrated luminosity profile. Extending outwards from the bulge is a fainter, disk-like component. Hints of spiral arm structure are subtle or non-existent, suggesting a relatively undisturbed morphology. The overall color appears reddish, indicative of an older stellar population. There is no obvious evidence of active star formation within the galaxy; light is dominated by redder wavelengths. There is no apparent distortion in the morphology, nor presence of tidal tails suggesting it is likely an isolated system and hasn't undergone any recent or major merger events. 
