The galaxy presents a largely smooth, elliptical morphology. It appears approximately round in shape, with a slight elongation possibly present but not definitively discernible due to the image resolution. The central region shows a concentrated, bright core that gradually diffuses outwards. There is a general lack of distinct features such as spiral arms or prominent dust lanes. The galaxy exhibits a color gradient, with the core appearing slightly redder than the outer regions. No significant tidal disturbances or merging signatures are readily apparent in the image, but close inspection suggests there is a minor disturbance present, perhaps from a gravitational interaction.
