The galaxy presents as a relatively compact object with an overall smooth morphology. The light distribution appears centrally concentrated, suggesting a possible elliptical or lenticular galaxy type. There is a slight elongation to the morphology. The galaxy exhibits a color gradient, with a brighter central region, possibly indicating an older stellar population. I do not see evidence of spiral arms or significant dust lanes. There are possible indications of minor disturbances or interactions; however, further analysis would be required to confirm this.
