The galaxy presents as an elongated, oval-shaped structure with a relatively smooth appearance. The light distribution suggests a central bulge that is more luminous than its surrounding regions. The galaxy exhibits a blueish hue, hinting at the presence of relatively young stars. Though a disk isn't distinctly visible, some irregularity can be seen. There appears to be an absence of prominent spiral arm structures or distinct dust lanes. The galaxy doesn't exhibit signs of a major ongoing merger, although some minor disturbance can't be ruled out. The galaxy lies at a redshift of approximately 0.101. Based on the appearance of this galaxy, its star formation rate is likely relatively low.