The galaxy presents an overall smooth morphology, with a dominant central bulge. The bulge exhibits a yellowish-white hue, indicative of an older stellar population. There is a hint of a fainter, bluer disk component surrounding the bulge. However, clear spiral arm structures are not apparent in this image. Some asymmetry is visible in the extended halo region of the galaxy, suggesting the possibility of minor tidal interactions or disturbances. A subtle reddish component is observed on one side, hinting at a region with either significant dust obscuration or a population of older, redder stars. The object appears to be actively star-forming based on color. Overall, this galaxy seems to be in a transitional stage, somewhere between a spiral and an elliptical morphology.
