The object appears to be a galaxy, exhibiting a relatively compact morphology. It presents as a slightly elongated structure, possibly indicative of a disk system viewed at a significant inclination. The central region is bright, suggesting a concentrated nucleus or bulge. The color profile displays a gradient, transitioning from a yellowish-white core to bluer outer regions. This may imply ongoing star formation in the spiral arms or outskirts, compared to an older stellar population in the central bulge. Some faint, irregular features are apparent, which may signify potential minor disturbances or interactions. The galaxy's appearance overall seems to be relatively undisturbed. 
