The galaxy presents as a centrally concentrated system with an overall smooth morphology. Its shape is somewhat elongated, with an axis ratio suggesting a possible elliptical form, although a highly inclined disk cannot be ruled out. The core region exhibits a bright, yellowish-orange hue, potentially indicative of an older stellar population. There is a faint extension of light surrounding the core and spanning the major axis, indicating a low surface brightness envelope. A region of slightly bluer light is seen on the upper left side of the image, suggesting ongoing or recent star formation. There does not appear to be a substantial amount of dust obscuration or evidence of strong spiral arm structures visible in this image. There are indications of some minor tidal disturbances, but they appear to be limited in scope.
