The galaxy exhibits a moderately concentrated light profile with an apparent angular size suggestive of a relatively compact structure. Morphologically, the galaxy presents an irregular appearance, possibly indicative of past or ongoing merger activity. The central region shows a higher concentration of light, and the overall structure appears to be in a transitional phase. There is a clear disk component. We see evidence of a recent merger. The color distribution suggests a diverse stellar population, with the redder colors dominating the central regions, perhaps indicating an older stellar population. Star formation is likely suppressed, as suggested by the redder colors in certain regions.
