The galaxy presents as a moderately luminous object with a generally smooth morphology. The central region exhibits a concentrated, brighter component that is yellowish in hue, suggesting a population of older stars. Surrounding this core is a more diffuse, bluish halo. The shape is elongated, neither perfectly spherical nor strongly disk-like. There is a suggestion of a slight tidal disturbance, perhaps indicating a past or ongoing minor interaction with another galaxy. Star formation appears to be present at a low level, given the presence of blue light, but is not dominant. Overall, the galaxy appears to be an intermediate mass object, consistent with a transitioning morphology between a spiral and elliptical galaxy.