The galaxy presents a predominantly smooth morphology, suggestive of an elliptical or lenticular type. The central region exhibits a high concentration of light, indicative of a significant stellar population and potentially an active galactic nucleus. The light from the central region has a slight red hue, possibly indicative of older stars. The galaxy's overall shape is moderately elliptical. There is little to no evidence of prominent spiral arms or a well-defined disk structure. No significant tidal features or signs of ongoing major mergers are observed; however, there are faint irregularities and blueish colors in the outer regions, implying a low level of recent star formation activity. These regions may have smaller populations of younger, hotter stars.
