The galaxy presents as a single, relatively smooth object with a centrally concentrated luminosity profile. Its morphology appears largely spheroidal, exhibiting a high degree of roundness. No prominent spiral arms, bars, or other distinct features are readily discernible. There is a lack of evidence for significant tidal disturbances or ongoing major merger activity. The galaxy exhibits a radial color gradient, appearing yellower in the core and transitioning to a slightly bluer hue in the outer regions. The overall color suggests a moderate population of older stars, though some level of ongoing star formation may be present. The object's size is moderately compact.
