The galaxy presents as an elongated, somewhat spindle-shaped structure. Its central region exhibits a higher surface brightness, appearing as a concentrated, diffuse glow. Moving outwards from the core, the light gradually diminishes, forming a fainter, more extended halo.

There is a subtle color gradient apparent. The central region displays a slightly redder hue, potentially indicative of an older stellar population. In contrast, the outer regions seem to possess a bluer tint, suggesting the presence of younger, hotter stars.

Overall, the galaxy appears relatively smooth and featureless. There are no obvious spiral arms, distinct dust lanes, or prominent star-forming regions readily visible within this image. Irregularities are minor, and disturbances from merging galaxies are not seen. The morphology of the galaxy indicates that it is a disk galaxy.
