The galaxy presents as an elliptical structure, seemingly lacking prominent spiral arms. The light distribution appears smooth with a centrally concentrated bulge, exhibiting a yellowish hue, possibly indicative of an older stellar population dominating the core. Moving outward from the core, the galaxy shows a gradual decrease in brightness. Faint hints of blue suggest some level of ongoing, or recent, star formation within the extended disk. The galaxy's overall morphology hints at a system that may have experienced, or is currently undergoing, minor interactions, as suggested by a subtle asymmetry in its outer regions.
