The galaxy presents as a centrally concentrated object, exhibiting a relatively smooth overall morphology. The central region displays a bright, yellowish-white core, suggesting the presence of an older stellar population and a potentially massive black hole accreting matter. The galaxy's light gradually diminishes from the core outwards, forming an extended halo. The shape appears close to round, with no prominent spiral arm structures or irregular features immediately discernible. There may be some subtle disc-like structure, but it is not immediately apparent. There is no obvious major or minor merging, and no significant tidal disturbance. The overall color index, inferred from the image's color balance, leans towards the redder end of the spectrum, indicating a population dominated by evolved stars and lower levels of ongoing star formation. The galaxy is relatively compact.
