The galaxy exhibits a generally smooth morphology, with a high degree of central concentration. It is roughly elliptical in shape, appearing nearly round with a slight elongation. The color gradient suggests a population of older stars, with a yellowish hue dominating the central region, potentially indicating a lower rate of recent star formation. There is very little evidence of spiral arm structure or distinct features that suggest a recent merger event, although there is a small visual distortion in the lower left quadrant. The galaxy appears to be a relatively undisturbed system.
