The galaxy presents as a single, concentrated object with a relatively smooth morphology. Its overall shape appears largely rounded, with minimal deviation from a circular form. A strong central bulge is evident, exhibiting a bright, concentrated luminosity that gradually fades towards the outer regions of the galaxy. No distinct spiral arm structures are discernible. The color profile suggests a more evolved stellar population, with a yellow/orange hue dominating the galaxy's light. There is no indication of ongoing major merging activity or significant tidal disturbances in the immediate vicinity of the galaxy. Evidence suggests that the rate of star formation is relatively low within this galaxy.
