The galaxy presents an elliptical morphology, exhibiting a smooth, diffuse light distribution. The central region appears brighter, suggesting a higher concentration of stars. The galaxy displays a slight elongation, appearing cigar-shaped. There is no apparent spiral arm structure or prominent dust lanes visible in the image. The overall color is yellowish, which suggests a stellar population dominated by older, redder stars and a relatively low rate of star formation. There is no obvious indication of any ongoing major merger events or tidal disturbances, though minor disturbances cannot be ruled out. The galaxy appears relatively isolated in this field.
