The galaxy presents as a relatively compact object with a somewhat smooth, elliptical morphology. There appears to be a subtle color gradient within the galaxy; its core exhibits a warmer, redder hue that graduates towards bluer, greener tones in the outer regions. It's difficult to discern any distinct structural features such as spiral arms or a prominent disk. There may be evidence of slight tidal disturbance or interaction, but it does not appear to be a major ongoing merger. Overall, the galaxy appears to be a relatively isolated system exhibiting moderate star formation activity.
