The galaxy presents as a centrally concentrated object with a generally smooth morphology. The central region appears bright and somewhat yellowish in color, indicative of a population of older stars. The galaxy appears nearly circular in shape. There is no obvious spiral structure or prominent disk features. It seems to be a relatively isolated system, showing no distinct signs of any ongoing major merger events or significant tidal disturbances. There might be the slightest indication of very faint and diffuse features but the resolution makes it challenging to determine if they are related to the galaxy itself.
