The galaxy appears as a moderately luminous object with a generally smooth morphology. It exhibits a slightly elliptical shape. Color gradients suggest a brighter, more concentrated central region with a yellowish hue, potentially indicating an older stellar population. There is a subtle color shift towards the outer regions which hints at bluer stars, but these are not strongly defined. The lack of prominent spiral arms or significant dust lanes suggests a relatively quiescent state regarding active star formation. There is a slight asymmetry to the galaxy's overall light distribution that could imply minor tidal interactions.
