The galaxy appears as a disk galaxy, viewed nearly edge-on from our line of sight. A prominent central bulge dominates the galaxy's core, exhibiting a smooth, concentrated luminosity profile, with yellow coloring which could indicate an older stellar population. The disk component is noticeably flattened and thin and shows some redder hues, perhaps due to dust extinction or older stars, and there is some faint bluish tinge near the rim of the disc, possibly indicating some star formation, though it is quite low. No signs of major interaction or tidal disturbance are visible in this image. The overall morphology suggests a relatively undisturbed, mature disk galaxy, possibly an Sa or Sb type.
