This galaxy presents as a relatively compact object with a high degree of central concentration. The core region exhibits a bright, yellowish-white hue, suggesting a population of older stars. Fainter material extends outwards, displaying a slightly irregular morphology with hints of a disturbed structure. A faint, diffuse arm-like feature is visible on one side, indicating potential interaction or tidal disruption. The overall color profile suggests ongoing, albeit moderate, star formation activity within the galaxy. There appears to be possible evidence of past or ongoing minor merger events in the system. The galaxy is neither perfectly elliptical nor a well-defined spiral, falling somewhere in between.
