The galaxy presents a primarily smooth morphology. The central region exhibits a concentrated and bright luminosity, indicative of a significant stellar population density and minimal dust obscuration. Extending outward from the core, the light fades gradually, forming an elliptical shape. The observed ellipticity suggests a potential for an oblate spheroidal structure, rather than a perfect sphere. There is a subtle color gradient from the central core, with the core being more white/yellow and the outer regions having a somewhat redder hue. There are no readily identifiable spiral arms, bars, or prominent dust lanes. The light distribution generally decreases smoothly from the center, supporting the classification of an elliptical-like galaxy. There are some blueish spots on the edges, suggesting some star formation may be occurring in the outer regions.
