The galaxy presents a generally smooth, elliptical morphology. It appears largely featureless, lacking prominent spiral arms or a distinct central bar structure. The light distribution is centrally concentrated with a gradual decrease in intensity moving outwards from the core. The color profile shows a dominant yellow hue, suggesting an older stellar population with a relatively low rate of ongoing star formation. There may be some evidence of minor tidal disturbance in the outer regions, indicating a possible past interaction or merger event, however these appear subtle and the overall structure is undisturbed. The round appearance of the object suggests a nearly face-on orientation relative to our line of sight.
