The galaxy presents an overall smooth appearance, with a generally elliptical morphology. There is a concentrated central bulge exhibiting a yellowish-orange hue, indicative of an older stellar population. Fainter, diffuse extensions emerge from this central region, showing a transition to cooler colors. These extensions suggest a less concentrated stellar distribution within the galaxy's outer regions. Some minor disturbances are visible in the galaxy's disk. Faint red components are observed, which may be H-alpha emission related to star formation.
