The galaxy presents a somewhat elongated, cigar-shaped morphology. The primary body appears relatively smooth in texture, with a centrally concentrated luminosity profile. The color distribution suggests an older stellar population, with a redder hue dominating the core and extended regions. There is faint evidence of bluer regions, possibly indicating areas of ongoing or recent star formation. No prominent spiral arm structures or a distinct disk component are discernible. There are hints of minor tidal disturbances or interactions, but it seems overall that this galaxy is not undergoing a major merger. 
