The galaxy presents as a moderately luminous, elongated structure. Its overall color appears to be dominated by reddish hues, suggesting an older stellar population, potentially with suppressed recent star formation. The morphology is primarily smooth, lacking prominent spiral arms or distinct features usually associated with actively star-forming regions. The central region exhibits a higher concentration of light, gradually fading towards the outer edges of the galaxy. The shape is definitively elongated, possibly a cigar shape, indicating an elliptical or lenticular morphology, without signs of any major disturbances or ongoing mergers. There may be very faint hints of a disk component.
