The galaxy presents as a moderately bright, relatively smooth object. Its morphology appears to be elliptical or lenticular based on the overall shape, exhibiting a lack of distinct spiral arms or prominent disk structures. There is an elongation visible, suggesting the galaxy is not perfectly spherical, but rather somewhat cigar shaped. The central region exhibits a brighter, more concentrated luminosity, likely indicating a nucleus or bulge. The color profile suggests a population of older stars, with a redder hue, however some star formation is still likely occurring. There is no clear evidence of recent major merger events, although minor disturbances or interactions with other galaxies cannot be completely ruled out based on this imagery alone.
