The galaxy exhibits a roughly elliptical morphology, appearing moderately compact with an angular extent of approximately 7 arcseconds. The central region displays a high surface brightness, exhibiting a bright, concentrated core. The color profile suggests a relatively blue stellar population in the central regions, transitioning to slightly redder hues in the outer regions. There is a hint of asymmetry or subtle disturbance in the structure, potentially indicating minor gravitational interactions or tidal effects. The outer regions appear somewhat diffuse, with no distinct spiral arm features immediately apparent. The light distribution is relatively smooth, however, there also appear to be minor artifacts. Further observations are necessary to confirm the nature and origin of these features.
