The galaxy presents a generally smooth and rounded morphology. Its light profile appears relatively even across the main body of the galaxy. There are no obvious spiral arms or a well-defined disk component. A central bulge region is subtly apparent, exhibiting a somewhat concentrated distribution of stellar light. The overall color appears to be trending towards the redder end of the spectrum, hinting at a population of older stars and potentially lower rates of ongoing star formation. There are no prominent features indicating a major ongoing merger event, though a very slight asymmetry is present in the galaxy’s shape, suggesting the potential for minor gravitational interactions in its past. 
