The galaxy presents as a singular, relatively smooth object, demonstrating a centrally concentrated luminosity profile. The morphology appears to be largely spheroidal, exhibiting a notable lack of distinct spiral arm structures or a prominent disk. The color index suggests a population dominated by older stars with a slightly reddish hue, potentially indicating lower levels of recent star formation activity. There is no strong evidence of ongoing mergers or tidal disturbances affecting the galaxy's overall structure. The galaxy has moderate luminosity.
