The galaxy presents an elongated, cigar-shaped morphology. A central bulge is visible, exhibiting a smooth light distribution with a yellowish-orange hue. A disk component is also present, extending beyond the bulge, though it appears relatively thin and somewhat indistinct. The color of the disk appears less red than the bulge. There's no clear indication of prominent spiral arms or active star-forming regions. The galaxy does not show significant signs of tidal disturbances or recent major merger events. The overall light profile suggests that the galaxy is likely a massive system, with a considerable population of older stars.
