The galaxy presents as a largely smooth, elliptical morphology. Its light profile appears centrally concentrated, fading gradually outwards with no distinct spiral arm structures or prominent dust lanes visible. The galaxy exhibits a yellowish-red hue, suggesting an older stellar population is dominant. There is no obvious central bulge. Its color and smoothness indicate a galaxy with little active star formation. Any ongoing star formation would be very low. There is also no evidence of any ongoing merger activity. The object exhibits an intermediate roundness, and is not obviously cigar shaped.
