The galaxy presents an overall elliptical morphology, appearing relatively smooth and concentrated towards the center. The central region exhibits a brighter, more luminous concentration, possibly indicative of an active galactic nucleus or a dense stellar population. The galaxy's shape is elongated, with an apparent cigar-like appearance. There is a subtle suggestion of a disk-like structure, but it is not clearly defined.

The galaxy displays a color gradient, transitioning from bluer hues in the central regions to slightly redder tones in the outer regions. The lack of significant dust lanes or prominent star-forming regions suggests that it is a relatively passive system with a low rate of star formation. There is a faint hint of a minor disturbance in the overall structure, which could indicate a past or ongoing minor interaction.