The galaxy presents an elongated, cigar-shaped morphology, appearing nearly edge-on. Its light distribution is relatively smooth, exhibiting a somewhat diffuse appearance across its structure. There is a suggestion of a slight color gradient along the major axis, with the central region exhibiting a yellowish hue that might suggest a population of older stars, while the outer regions have a slightly bluer tinge indicative of star formation. No spiral arm structures or prominent dust lanes are readily discernible. Overall, the galaxy appears undisturbed, lacking evidence of any major merger events or strong tidal interactions.
