The galaxy presents as a somewhat irregular, extended object. There is a subtle clumpy morphology with hints of spiral arms, though no grand design is apparent. The color profile suggests a relatively old stellar population, with a dominant reddish-yellow hue. There are a few brighter point-like sources embedded within the galaxy's disk, which may be star-forming regions or superclusters. However, there is likely an overall low star formation rate occurring in this galaxy. There is evidence of minor disturbances, potentially indicative of a past or ongoing interaction with a smaller galaxy or tidal effects from the intergalactic medium. The galaxy appears to be relatively massive. The central region shows an increase in brightness and density.
