The galaxy appears to be an elliptical type, exhibiting a generally smooth, featureless morphology. Its overall shape is elongated, approaching a cigar-like form, with the major axis appearing significantly longer than the minor axis. The light distribution is concentrated towards the center, suggesting a dense galactic nucleus. There is no apparent spiral structure or distinct dust lanes. A slight color gradient can be observed, with the central region exhibiting a whiter, possibly slightly bluer hue than the outer regions, which show a tendency towards redder tones. There appears to be only a slight disturbance visible, which may indicate a minor interaction.
