The galaxy presents as a centrally concentrated, generally smooth structure. The central region exhibits a bright, yellowish hue, suggesting an older stellar population. Moving outwards from the core, the galaxy transitions to a more diffuse, greenish-tinged halo, possibly indicating a region of ongoing, albeit subdued, star formation activity. The overall shape approximates a slightly elongated ellipse, appearing more rounded than cigar-shaped. There is no apparent evidence of a spiral disk or distinct spiral arms. Faint indications suggest a possible minor disturbance in the outer regions, but no major merging activity or tidal tails are readily visible. The galaxy appears largely isolated.
