The galaxy presents as a generally smooth, elongated form. The light is concentrated in the center, which appears to be its brightest region. The galaxy exhibits a gradient, decreasing in luminosity from the center towards the edges. There is an indication of a slight disturbance or feature emanating from the central region, possibly indicative of a minor interaction or internal activity. It appears to be more cigar shaped than circular. Overall, the galaxy's morphology suggests that it is not currently undergoing major merger activity. The distribution of light suggests that star formation is not particularly intense within this galaxy.
