The galaxy presents as a relatively smooth, cigar-shaped structure with a defined central bulge. The color profile suggests a dominant population of older stars concentrated in the core, exhibiting a reddish-orange hue. Extending outwards from this central region, a bluer halo is visible, hinting at more recent star formation activity. No distinct spiral arms or strong dust lanes are apparent within the visible light spectrum. There's no obvious indication of on-going major merger activity, although there's some minor disturbances. The overall morphology is that of a relatively evolved system. The galaxy is estimated to be of intermediate mass with a moderate star formation rate.
