The galaxy exhibits a generally smooth morphology, with a slightly elongated, cigar-like shape. The central region appears more luminous, showing a concentration of older stars, indicated by the yellowish hue. Moving outward from the center, a subtle blue-ish tint is apparent, particularly in the outer regions, which may imply the presence of some younger stellar populations or ongoing, albeit low, star formation. No distinct spiral arms or a bar structure are clearly visible. Faint disturbances or tidal features are not evident, suggesting it hasn't undergone recent major mergers. The galaxy presents a relatively undisturbed structure. 
