The galaxy presents as a relatively smooth, centrally concentrated object. It appears largely elliptical in shape, exhibiting a high degree of roundness in its overall morphology. There is no discernible disk structure or spiral arm features. The galaxy's light profile indicates a generally homogenous stellar population distribution. The object does not show any signs of ongoing major merging activity or significant tidal disturbances. In terms of color, the galaxy displays a somewhat red-shifted appearance. This redness indicates a potentially older stellar population and low levels of current star formation activity. There is no apparent active galactic nucleus or prominent dust lanes visible.
