The galaxy exhibits a somewhat elliptical morphology, appearing neither perfectly spherical nor a well-defined spiral. The central region is characterized by a bright, concentrated luminosity, suggesting a significant stellar population density and likely an older stellar population. The color of this central bulge appears yellowish, indicative of evolved stars. 

Surrounding the central region, there is a fainter, more diffuse halo. This outer region displays some subtle, irregular features. The color gradients within this halo suggest a mix of stellar populations. There are faint hints of blueish regions, possibly indicating areas of recent or ongoing star formation, though the overall star formation rate appears to be relatively low. A slight tidal tail is present, possibly indicating past or ongoing interactions with another galaxy.
