The galaxy presents as a somewhat elliptical structure, displaying a generally smooth appearance across the main body. The central region exhibits a brighter, more concentrated luminosity, suggesting a possible central bulge. Faint color gradients are observable, with the central region tending towards a yellowish hue, potentially indicative of an older stellar population. A secondary, slightly detached component is visible, appearing more compact and with a reddish tint, possibly a satellite galaxy or a region of active star formation within the same system. The overall shape is neither perfectly spherical nor highly elongated, representing an intermediate form. There is a suggestion of mild distortion or tidal features, hinting at a possible past or ongoing interaction.
