The galaxy presents an elliptical morphology, appearing as a cigar-shaped structure. The central region exhibits a bright, concentrated luminosity indicative of a prominent galactic nucleus or bulge. The overall color profile suggests a population of older stars with a redder hue. There may be a small amount of ongoing star formation. The galaxy shows minimal signs of disturbance or interaction with other galaxies and has a relatively smooth, indistinct structure without well-defined spiral arms or other distinct features.
