The observed galaxy exhibits a predominantly smooth morphology, suggesting an elliptical or lenticular classification. Its overall shape appears somewhat rounded, with a slight deviation toward an intermediate form, rather than a perfectly circular or elongated structure. The galaxy displays a yellow-white hue at its core, indicative of an older stellar population. There are subtle indications of a disk, but it is very minor and more likely to be light from the core. No strong signs of recent or ongoing merger activity are apparent; however, there are no visible spiral arms or significant dust lanes. Given the red shift data, it seems to be approximately 2.6 kpc in size. Further spectroscopic analysis is needed to confirm this preliminary morphological assessment and analyze the star formation activity.
