The galaxy presents as a generally smooth object, exhibiting a concentrated central bulge. A faint, extended halo surrounds the central region, appearing less structured and gradually fading into the background sky. The color profile shows a yellowish core, indicative of an older stellar population. There is very little evidence of prominent spiral arm structure or dust lanes. Overall, the morphological characteristics suggest a classification leaning towards an elliptical galaxy or a lenticular galaxy with minimal ongoing star formation. There may be some slight irregularities that suggest a potential merger in the distant past.
