The galaxy presents a smooth, elongated morphology, consistent with an elliptical type. The light distribution is centrally concentrated, with a gradual decrease in intensity towards the outer regions. No distinct spiral arms or prominent dust lanes are discernible. The overall color appears to be a slightly blueish hue, suggesting a population of younger stars and active star formation, although the smoothness of the profile indicates that any disk component is minimal. The major axis of the galaxy is significantly longer than the minor axis, indicating a cigar-like shape. There appears to be a minor tidal disturbance, possibly resulting from a past interaction with another galaxy, although this is very faint. There is no current merging activity visible.
