The galaxy presents as a somewhat elongated, elliptical structure with a bright, concentrated central bulge. The bulge exhibits a reddish-orange hue, potentially indicating an older stellar population. Surrounding the bulge is a fainter, more diffuse disk-like component displaying a greenish tint. This coloration might be suggestive of ongoing, albeit relatively low, star formation within this region. There's no distinct spiral arm structure visible. The galaxy's overall shape is somewhat cigar-shaped, appearing longer than it is wide. It does not show any obvious signs of major disturbances or mergers.
