The galaxy presents as a concentrated, luminous object with a generally smooth morphology. The primary light source appears to emanate from a central region displaying a yellowish hue, suggesting an older stellar population. The shape approximates a slightly elongated ellipse. There is evidence of fainter, bluer light surrounding this core, concentrated in clumps that may indicate regions of more recent star formation. There appears to be evidence of possible tidal disruption or interaction, and the general asymmetry suggests an ongoing or recent merger event. 
