The galaxy presents as a disk galaxy, likely viewed at a high inclination. There is evidence of a central bulge component, exhibiting a yellowish-white hue, with an extended disk showing a bluer color profile. The disk appears relatively smooth, with a possible hint of spiral arm structure beginning to emerge. No significant dust lanes or strong star-forming regions are immediately apparent, suggesting a low to moderate star formation rate, with a high likelihood that the star formation is suppressed. The galaxy does not appear to be undergoing any major merging events or tidal disruptions.
