The galaxy presents as a single, distinct object exhibiting an apparent disturbed morphology. It is neither purely elliptical nor a well-defined spiral; rather, it shows irregular features suggesting possible interaction or recent merger activity. The central region appears brighter and more concentrated, surrounded by a fainter, extended halo.

A color gradient is visible across the galaxy. The central region displays a bluer hue, indicating the presence of younger, hotter stars and active star formation. Conversely, the outer regions trend towards a redder color, suggesting an older stellar population. There also appears to be evidence of dust lanes. Overall, this galaxy shows a moderately low redshift.
