The galaxy presents as a moderately luminous object with a relatively smooth and rounded morphology. There is no clear evidence of spiral arm structure or a prominent disk component; instead, the light is concentrated in a central region that gradually fades outwards. The galaxy appears roughly elliptical, with a notable lack of any significant tidal disturbances or ongoing merger activity. The color profile suggests a population of older stars, emitting light predominantly at the redder end of the spectrum, giving the galaxy a yellow hue. This may indicate a lower current rate of star formation.
