The galaxy presents as an elongated, spindle-shaped structure, viewed at a high inclination. A prominent central bulge is evident, displaying a yellowish-orange hue, likely indicative of an older stellar population. Extending outwards from the bulge, the galactic disc exhibits a bluer color gradient, which suggests the presence of younger, hotter stars and ongoing star formation in these regions. There are no obvious spiral arm features. The galaxy appears relatively isolated. The morphology does not show evidence of recent or ongoing major merger events. The observed redshift suggests the galaxy is relatively distant.
