The galaxy appears to be a relatively compact system, exhibiting a predominantly smooth morphology. There is a slight elongation, but generally presents as moderately rounded. The color profile is consistent with an evolved stellar population. A subtle central concentration is visible with a gradual decline in luminosity outwards. There appears to be some minor disturbance in its morphology, possibly a faint tidal feature suggesting a past or ongoing interaction. No prominent spiral arms or dust lanes are discernible, suggesting the galaxy is relatively quiescent in terms of active star formation.
