The galaxy presents a moderately inclined disk structure. There is evidence of spiral arm structure; however, it's somewhat faint and flocculent, not tightly wound. The central bulge region appears prominent and relatively bright with a smooth, concentrated light distribution. The color profile suggests a mix of stellar populations, with the bulge perhaps exhibiting a slightly redder hue indicating older stars, compared to the bluer tints observed in the disk, which potentially signify ongoing star formation. The overall morphology leans towards a transition between a purely elliptical galaxy and a well-defined spiral. There are hints of minor disturbances or asymmetries in the outer disk, possibly resulting from gravitational interactions, although no major merger is immediately apparent. The galaxy exhibits a diffuse halo or extended component, suggesting a relatively large size.
