The galaxy presents as a slightly elongated, lenticular or elliptical structure. Its color profile suggests a more evolved stellar population, exhibiting a yellowish-red hue characteristic of older stars. The overall light distribution is smooth and centralized, with a relatively high surface brightness. There are no prominent spiral arms or dust lanes visible, indicating a lack of significant ongoing star formation. The galaxy appears mostly undisturbed, showing no signs of a major merger event. A slight asymmetry or minor disturbance is possible, but not definitively discernible from the available data. The shape leans more towards a cigar-like form than a perfectly round one.
