The galaxy exhibits a generally smooth morphology, with a near absence of distinct spiral arms or prominent dust lanes. The light distribution is concentrated towards the center, indicating a prominent bulge. The object appears somewhat elliptical in shape, displaying a slight elongation rather than a perfectly circular form. The color profile suggests a relatively evolved stellar population, with a yellowish hue dominating the central region. There may be a faint hint of bluer tones in the outer edges of the galaxy, which might indicate more recent star formation in these regions, but these are not easily discerned. There is no obvious evidence of a major ongoing merger event. The overall appearance indicates a galaxy which may be a disk galaxy or elliptical galaxy with limited ongoing star formation.
