The galaxy presents as a relatively smooth, elongated object, appearing cigar-shaped. Its light distribution is concentrated centrally with a gradual decrease in intensity towards the outer edges, suggesting a high degree of central mass concentration. The galaxy exhibits a blue hue, indicative of a relatively younger stellar population and ongoing star formation. There are no distinct spiral arms or prominent dust lanes visible. The lack of clear features supports a classification as an elliptical or lenticular galaxy type, though deeper imaging would be required to confirm the classification and to rule out the presence of subtle structural details. Based on the overall smoothness, the galaxy does not appear to be undergoing any major merging or tidal disturbances.
