The galaxy appears to be an elliptical type, exhibiting a generally smooth morphology. The central region presents a bright, concentrated luminosity gradient. The galaxy shows an overall yellowish hue, possibly indicative of an older stellar population. There is a slight hint of some bluer emission in the outskirts indicating possible star formation. The shape is roughly elliptical, with an apparent axis ratio that suggests a relatively small amount of flattening, and it appears to have only minor disturbances. There are no obvious spiral arms or a prominent disk component.
