The galaxy presents a morphology consistent with a spiral type, viewed at a slight angle relative to edge-on. The galaxy exhibits a discernible disk component, with evidence of spiral arm structures, although the resolution limits detailed tracing. A central bulge is visible, appearing moderately sized in relation to the disk.

Color gradients suggest varying stellar populations and dust distribution. The central region displays a slightly redder hue, potentially indicating older stellar populations and/or dust obscuration. A hint of bluer regions within the disk may indicate ongoing star formation activity. The presence of bar structure is ambiguous.

Overall, this galaxy presents characteristics expected of a spiral galaxy undergoing active star formation. There are no indications of an advanced merger or strong tidal disturbances.
