The galaxy presents as a relatively smooth, elongated structure, approximately 4 kpc in effective radius. Its overall shape is notably cigar-shaped, lacking any discernible spiral arms or prominent features indicative of a disk galaxy. The galaxy exhibits a central concentration of light, suggesting the presence of a bulge component. The color profile appears consistent across the galaxy, with a general trend towards redder hues, indicative of a stellar population that is either older or dust-obscured. There is no visual evidence of active star formation regions or tidal disturbances. It's classified morphologically as a likely elliptical galaxy exhibiting minimal signs of recent interaction or merging activity.
