The galaxy presents a generally smooth morphology, appearing elongated or cigar-shaped in its overall form. Its light is dominated by warmer hues, trending toward orange-yellow, suggestive of an older stellar population. There is minimal indication of spiral arm structure or patchy blue regions indicating ongoing star formation. The central region is bright, indicating a concentration of stars. There appears to be no major merging activity. Based on the color, the galaxy appears to have a relatively low star formation rate.
