The galaxy presents a somewhat elliptical morphology, suggestive of a disk galaxy viewed at an angle. Its color appears generally yellowish-red, with the central bulge region exhibiting a brighter, more concentrated light distribution, which could indicate an older stellar population and a lack of significant ongoing star formation. The disk component is fainter and less well-defined, hinting at either a relatively low surface brightness or the presence of dust obscuration. No prominent spiral arms or distinct features such as star-forming regions are readily apparent, leading to a classification of a potentially smooth galaxy. The overall appearance suggests the possibility of a low rate of star formation. There may be some minor disruption of the edges of the galaxy, possibly indicating a minor disturbance.
